Pith. sign in

REVIEW 2 major objections 2 minor 297 references

Accretion of Primordial Black Holes in Stellar Interiors

T0 review · 2 major / 2 minor · reviewed 2026-06-28 · grok-4.3

Challenge this review Re-run · record.json Download PDF Read on arXiv ↗

Pith's one-line read Cooling near the event horizon lets primordial black holes as light as 10^{-16} solar masses consume a solar-mass star within a Hubble time.

desk verdict The paper delivers a self-consistent numerical determination of radiative efficiency for PBH accretion that lowers the critical mass for stellar consumption. read the letter →

arxiv 2606.02726 v1 pith:2BU6AEFQ submitted 2026-06-01 astro-ph.HE astro-ph.SR

Matteo Cantiello , Ore Gottlieb , Cameron Norton , Matthew Kleban , Ken Van Tilburg This is my paper · ORCID
classification astro-ph.HEastro-ph.SR
keywords primordialblackholesstellaraccretionBondiradiativeefficiencybremsstrahlungcoolingphotontrappingregimes
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

The paper computes how small primordial black holes accrete gas while embedded in the core of a sun-like star, solving the flow equations with self-consistent cooling for the first time. It shows that bremsstrahlung radiation at temperatures near 10^{11} K near the black hole changes the accretion from the classical adiabatic case, raising the mass inflow rate by a factor of 2 to 7 and dropping the fraction of rest-mass energy radiated away by roughly ten times. These changes keep the growth super-exponential across three identified regimes and lower the starting mass needed for the black hole to swallow the entire star in cosmic time to about 10^{-16} solar masses. A reader would care because the result revises how dangerous or detectable such black holes could be inside ordinary stars.

What carries the argument

Time-dependent spherical Euler equations with an implicit cooling source term that self-consistently sets the accretion rate and radiative efficiency in three regimes from Hot Bondi through bremsstrahlung cooling to photon trapping.

What would settle it

A simulation of the same mass range that includes explicit radiative transfer and shows the accretion rate or efficiency differing by more than a factor of two from the values reported for masses near 10^{-16} solar masses.

Watch

Extended reading notes

Core claim

We solve the time-dependent spherical Euler equations with an implicit cooling source term to determine accretion rate, radiative efficiency, and flow structure self-consistently across the optically thin range. This yields three regimes: a Hot Bondi regime below 10^{-14} solar masses where cooling is negligible; a bremsstrahlung-cooling regime from 10^{-14} to 5 times 10^{-13} solar masses that drives the flow toward isothermal with efficiency near 10^{-2}; and a photon-trapping regime above that mass where the Bondi sphere is optically thick and the rate stays near the classical Bondi value. Cooling therefore enhances the accretion rate by a factor of roughly 2-7 throughout the spherical r

Load-bearing premise

Microphysical cooling at temperatures around 10^{11} K can be captured by an implicit source term in the spherical Euler equations without needing full radiation transport or magnetic fields.

Editorial extensions

If this is right

  • Growth of the black hole remains super-exponential while the flow stays spherical.
  • Radiative efficiency falls to approximately 10^{-2} once bremsstrahlung cooling becomes important.
  • Above 5 times 10^{-13} solar masses the accretion rate stays close to the classical Bondi value because of photon trapping.
  • The threshold mass for destroying a solar-mass star drops to roughly 10^{-16} solar masses.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • Stellar lifetimes could place new upper limits on the abundance of primordial black holes if the cooling-enhanced growth holds.
  • The same cooling physics might alter accretion estimates for other compact objects embedded in dense gas.
  • Observing unusually rapid stellar evolution or sudden disappearance of stars could test the predicted growth rates.
Share X Bluesky LinkedIn Reddit HN

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit.

Referee Report

2 major / 2 minor

Summary. The paper studies spherical accretion of primordial black holes (PBHs) in solar-type stellar cores. It solves the time-dependent spherical Euler equations with an implicit cooling source term to compute radiative efficiency self-consistently in the optically thin regime (10^{-16.5} to 10^{-10} M_⊙), then switches to an analytical photon-trapping prescription above 5×10^{-13} M_⊙. The work identifies three regimes (Hot Bondi, bremsstrahlung-cooling, photon-trapping), finds cooling enhances \dot M by a factor of ~2-7 with η≈10^{-2}, and concludes the critical initial PBH mass to consume a solar-mass star in a Hubble time is M_{0,crit}∼10^{-16} M_⊙.

Significance. If the numerical results hold, the self-consistent treatment of cooling and efficiency across regimes strengthens constraints on PBH masses that could disrupt stars, with implications for PBH dark matter searches. The time-dependent simulations determining \dot M and η without post-hoc fitting are a methodological strength relative to prior analytic Bondi assumptions.

major comments (2)
  1. [description of bremsstrahlung-cooling regime and implicit cooling implementation] The bremsstrahlung-cooling regime (10^{-14} to 5×10^{-13} M_⊙) relies on an implicit cooling source term in the Euler equations to produce the factor of 2-7 enhancement in \dot M and the drop in η to ~10^{-2}; this term replaces full radiation transport near r_S at T~10^{11} K where optical depth nears unity, but the manuscript provides no quantitative test (e.g., comparison to diffusion approximation or optical-depth calculation) showing the net cooling rate is accurate to better than the reported enhancement factor.
  2. [transition to photon-trapping regime] The switch to the analytical photon-trapping prescription at exactly 5×10^{-13} M_⊙ is presented as the point where the Bondi sphere becomes optically thick, yet this threshold is listed among the free parameters and lacks an explicit derivation from the simulated optical depth or trapping condition; altering it would directly rescale the integrated growth and shift M_{0,crit}.
minor comments (2)
  1. Notation for the three regimes should be defined once with explicit mass boundaries and referenced consistently when quoting the enhancement factor.
  2. The abstract states the enhancement keeps growth 'super-exponential throughout the spherical regime'; a brief quantitative comparison of the integrated growth timescale with and without cooling would clarify this claim.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their careful review and for recognizing the methodological value of our time-dependent simulations. We respond to the major comments below and will revise the manuscript to address the identified gaps in validation and derivation.

read point-by-point responses

  1. Referee: The bremsstrahlung-cooling regime (10^{-14} to 5×10^{-13} M_⊙) relies on an implicit cooling source term in the Euler equations to produce the factor of 2-7 enhancement in \dot M and the drop in η to ~10^{-2}; this term replaces full radiation transport near r_S at T~10^{11} K where optical depth nears unity, but the manuscript provides no quantitative test (e.g., comparison to diffusion approximation or optical-depth calculation) showing the net cooling rate is accurate to better than the reported enhancement factor.

    Authors: We agree that a quantitative validation of the implicit cooling term would strengthen the results. The term is used because the cooling timescale is much shorter than the dynamical timescale in this regime, but we will add to the revised manuscript an explicit optical-depth calculation using the simulated density and temperature profiles near r_S, together with a comparison of the cooling rate to the diffusion approximation. This will confirm that the reported enhancement remains robust. revision: yes

  2. Referee: The switch to the analytical photon-trapping prescription at exactly 5×10^{-13} M_⊙ is presented as the point where the Bondi sphere becomes optically thick, yet this threshold is listed among the free parameters and lacks an explicit derivation from the simulated optical depth or trapping condition; altering it would directly rescale the integrated growth and shift M_{0,crit}.

    Authors: The threshold marks the mass at which the simulated Bondi sphere reaches optical depth of order unity. While the original text did not include the explicit derivation, the value is physically motivated rather than arbitrary. In revision we will add the optical-depth calculation versus black-hole mass extracted from the simulations to derive the transition point, and we will include a sensitivity test showing the effect of varying the threshold on the integrated growth and on M_{0,crit}. revision: yes

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity; central results from self-consistent simulations

full rationale

The paper computes radiative efficiency, accretion rates, and the critical PBH mass M_{0,crit} via time-dependent spherical Euler simulations with an implicit cooling term across the optically thin regime, followed by an analytic photon-trapping model above 5e-13 M_sun. These steps determine \dot M and \eta directly from the equations without any reduction to a fitted parameter defined from the target result, self-citation load-bearing the central claim, or ansatz smuggled via prior work. The derivation chain remains independent of the final M_{0,crit} value.

Assumptions & free parameters 2 free parameters · 2 assumptions · 0 invented entities

The central claim rests on standard hydrodynamics plus specific microphysical cooling rates at extreme temperatures; no new particles or forces are introduced, but several modeling choices function as effective free parameters.

free parameters (2)
  • transition mass for photon-trapping prescription
    The switch at 5e-13 M_sun from simulation to analytic treatment is chosen to match optical depth; its exact value affects the quoted growth factor.
  • implicit cooling implementation details
    The precise form of the cooling function (bremsstrahlung coefficient, temperature dependence) is not stated and must be assumed from standard tables.
assumptions (2)
  • domain assumption Spherical symmetry and absence of magnetic fields or angular momentum remain valid throughout the accretion flow
    Invoked when the authors restrict the problem to the time-dependent spherical Euler equations.
  • domain assumption Microphysical radiative processes at T~10^11 K near r_S can be treated as an optically thin cooling term without full radiative transfer
    Required for the self-consistent eta calculation in the optically thin regime.

how reviews work

0 comments
Cite this review

Pith. "Pith review of Accretion of Primordial Black Holes in Stellar Interiors." pith.science (2026). https://pith.science/paper/2BU6AEFQ

@misc{pith2026260602726,
  author       = {Pith},
  title        = {Pith review of: Accretion of Primordial Black Holes in Stellar Interiors},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/2BU6AEFQ}},
  note         = {Machine review of arXiv:2606.02726}
}
abstract

We study spherical accretion onto primordial black holes (PBHs) embedded in the core of a solar-type star. We compute the radiative efficiency self-consistently for the first time across the optically thin range ($10^{-16.5}$-$10^{-10}M_\odot$) with time-dependent simulations, and follow the growth up to $10^{-2}M_\odot$ using an analytical photon-trapping prescription above $5\times 10^{-13}M_\odot$. Near the Schwarzschild radius ($r_{\rm S}\sim 10^{-11}$cm for a $10^{-16}M_\odot$ PBH), gas compressed to $T\sim 10^{11}$K radiates through microphysical processes that fundamentally alter the classical adiabatic Bondi solution. We solve the time-dependent spherical Euler equations with an implicit cooling source term, determining $\dot M$, $\eta = L/\dot M c^2$, and the flow structure self-consistently. We identify three regimes for spherical accretion: a Hot Bondi regime ($M_{\rm BH}\lesssim 10^{-14}M_\odot$) in which bremsstrahlung cooling is dynamically negligible; a bremsstrahlung-cooling regime ($10^{-14}$-$5\times 10^{-13}M_\odot$) driving the flow toward isothermal with $\eta\approx 10^{-2}$; and a photon-trapping regime above $5\times 10^{-13}M_\odot$, in which the Bondi sphere is optically thick and the accretion rate remains close to the Bondi value. Cooling enhances $\dot M$ by a factor of $\sim$2-7, keeping growth super-exponential throughout the spherical regime. The radiative efficiency is an order of magnitude lower than previously assumed, and the critical initial PBH mass required to consume a solar-mass star within a Hubble time is $M_{\rm 0,crit}\sim 10^{-16}M_\odot$.

Figures

Figures reproduced from arXiv: 2606.02726 by the authors.

Figure 1
Figure 1. Schematic of the radiative feedback mechanism on the Bondi boundary conditions. Accretion luminosity Lacc produced near the PBH (central black circle) escapes the Bondi sphere (blue circle, radius rB) and is absorbed by the ambient stellar plasma just outside it, raising the local temperature from T∞ to T∞ + ∆T (or￾ange shading). The deposited energy is transported outward by pho￾ton diffusion (brown dashed arrows) … view at source ↗
Figure 2
Figure 2. Schematic overview of the three spherical-accretion regimes and the disk-accretion regime onto a PBH embedded in a stellar interior, ordered by increasing MBH. Hot Bondi (MBH ≲ 10−14 M⊙): the Bondi sphere is optically thin (τ < 1); bremsstrahlung photons (orange wavy arrows) escape freely without interacting with the infalling gas (grey arrows), yielding η ≈ 10−2 . Bremsstrahlung cooling (10−14–5×10−13 M⊙): bremsstr… view at source ↗
Figure 3
Figure 3. Physical length scales controlling the accretion regime as a function of PBH mass, for solar core conditions. The Bondi ra￾dius rB (blue) defines the gravitational sphere of influence. The vertical dotted line marks τ(rB) = 1, where the Bondi sphere becomes optically thick (M ∼ 5 × 10−13 M⊙). The photon trapping radius rtrap (red) exceeds rB at M ∼ 10−9 M⊙. Two circularization radii rcirc (or￾ange) are shown: one fo… view at source ↗
Figures from the paper (7 more)
Figure 4
Figure 4. Figure 4: Steady-state radial profiles from the time-dependent Euler solver for MBH = 10−16, 10−13, and 10−11 M⊙. (a) Temperature, (b) infall velocity, (c) density, and (d) Mach number as a function of r/rS. Dashed grey lines show the adiabatic Bondi solution. The vertical dashe…
Figure 5
Figure 5. Figure 5: Opacity (top) and cumulative optical depth (bottom) as a function of r/rS for MBH = 10−16, 10−13, and 10−11 M⊙. Thick translucent lines show the total opacity; dashed lines show Klein–Nishina–corrected scattering; dotted lines show Kramers free–free absorption. The ver…
Figure 7
Figure 7. Figure 7: Accretion luminosity as a function of BH mass. The solid blue line shows the locally emitted luminosity Lemitted = η M c ˙ 2 evaluated with the cooling-enhanced accretion rate; the dotted blue line shows the bare-Bondi reference η M˙Bc 2 without the cool￾ing enhancemen…
Figure 8
Figure 8. Figure 8: Top panel: Accretion rate onto a PBH in the solar core as a function of BH mass. The gray solid line shows the adiabatic Bondi rate M˙B ∝ M2 ; the blue dashed line shows the isothermal-limit cooling-enhanced rate f(M)M˙B; the red dotted line shows the legacy Eddington …
Figure 9
Figure 9. Figure 9: Growth trajectories MBH(t) for PBHs with initial masses M0 = 10−17–10−10 M⊙ embedded in the solar core (color scale, from light to dark green). Trajectories are trimmed at 0.01M⊙. PBHs with M0 ≳ 10−16 M⊙ reach this threshold within a Hubble time; lighter PBHs stall in …
Figure 10
Figure 10. Figure 10: Schematic of the recycling/pile-up geometry inside the collisionless region. The flow is hydrodynamic near rB and becomes collisionless below rcoll. Most particles miss the GR loss cone on a single inward pass, return to rcoll, re-thermalize, and either are recaptured…
Figure 11
Figure 11. Figure 11: Effective Knudsen number at the circularization radius as a function of specific angular momentum, for MBH = 10−16 M⊙. The hatched bands mark the excluded loss-cone (ℓ < ℓcrit) and reflected (ℓ > ℓmax) populations. The pile-up enhancement ξ (ℓ) is sufficient to make K…

Discussion (0). Continue with ORCID to comment.

Reference graph

Works this paper leans on

297 extracted references · 265 canonical work pages

  1. [1]

    The Internal Constitution of the Stars

  2. [2]

    , year = 1957, month = jan, volume =

    Statistical dynamics and accretion. , year = 1957, month = jan, volume =. doi:10.1093/mnras/117.1.50 , adsurl =

    work page doi:10.1093/mnras/117.1.50 1957

  3. [3]

    , keywords =

    Nearly collisionless spherical accretion. , keywords =. doi:10.1093/mnras/181.2.347 , adsurl =

    work page doi:10.1093/mnras/181.2.347

  4. [4]

    Improved angular momentum evolution model for solar-like stars

    Improved angular momentum evolution model for solar-like stars. , keywords =. doi:10.1051/0004-6361/201321302 , archivePrefix =. 1306.2130 , primaryClass =

    work page Pith review arXiv doi:10.1051/0004-6361/201321302

  5. [5]

    , year = 1959, month = feb, volume =

    Spontaneously Growing Transverse Waves in a Plasma Due to an Anisotropic Velocity Distribution. , year = 1959, month = feb, volume =. doi:10.1103/PhysRevLett.2.83 , adsurl =

    work page doi:10.1103/physrevlett.2.83 1959

  6. [6]

    , keywords =

    Nonadiabatic self-consistent spherical accretion as a model for quasars and active galactic nuclei. , keywords =. doi:10.1086/162175 , adsurl =

    work page doi:10.1086/162175

  7. [7]

    , keywords =

    Stationary spherical accretion into black holes - The transition from the optically thin to the optically thick regime. , keywords =

  8. [8]

    , keywords =

    Resonant Enhancements in Weakly Interacting Massive Particle Capture by the Earth. , keywords =. doi:10.1086/165653 , adsurl =

    work page doi:10.1086/165653

Show all 297 references
  1. [9]

    , keywords =

    Capture by the sun of a galactic population of weakly interacting, massive particles. , keywords =. doi:10.1086/163485 , adsurl =

    doi

  2. [10]

    , keywords =

    Accretion of Matter by Condensed Objects. , keywords =. doi:10.1007/BF00649949 , adsurl =

    doi

  3. [11]

    , keywords =

    Radiation from spherical accretion onto black holes. , keywords =

  4. [12]

    , year = 1973, month = mar, volume =

    Accretion onto Black Holes: the Emergent Radiation Spectrum. , year = 1973, month = mar, volume =. doi:10.1086/151982 , adsurl =

    1973 doi

  5. [13]

    , keywords =

    Super-Eddington Accretion onto Black Holes and Its Application to Fallback Accretion. , keywords =. doi:10.3847/1538-4357/ae30dc , archivePrefix =. 2507.16893 , primaryClass =

    doi

  6. [14]

    , keywords =

    Black holes in radiation-dominated gas: an analogue of the Bondi accretion problem. , keywords =. doi:10.1093/mnras/184.1.53 , adsurl =

    doi

  7. [15]

    I - Equations and numerical methods

    Optically thick, time-dependent spherical accretion onto a black hole. I - Equations and numerical methods. , keywords =. doi:10.1086/162419 , adsurl =

    doi

  8. [16]

    III Optically thick accretion in particular cases

    Stationary spherical accretion into black holes. III Optically thick accretion in particular cases. , keywords =. doi:10.1093/mnras/206.3.589 , adsurl =

    doi

  9. [17]

    Self-consistent Models of Spherical Accretion onto Black Holes. II. Two-Temperature Solutions with Pairs. , keywords =. doi:10.1086/168669 , adsurl =

    doi

  10. [18]

    , keywords =

    Spherical Accretion onto Black Holes: A Complete Analysis of Stationary Solutions. , keywords =. doi:10.1086/170781 , adsurl =

    doi

  11. [19]

    Rubin, S. G. and Khlopov, M. Yu. and Sakharov, A. S. Primordial black holes from nonequilibrium second order phase transition. Grav. Cosmol. 2000. arXiv:hep-ph/0005271

    2000 arXiv

  12. [20]

    Black holes and the multiverse , volume=

    Garriga, Jaume and Vilenkin, Alexander and Zhang, Jun , year=. Black holes and the multiverse , volume=. Journal of Cosmology and Astroparticle Physics , publisher=. doi:10.1088/1475-7516/2016/02/064 , number=

    2016 doi

  13. [21]

    Spontaneous Generation of Density Perturbations in the Early Universe

    Crawford, Matt and Schramm, David N. Spontaneous Generation of Density Perturbations in the Early Universe. Nature. 1982. doi:10.1038/298538a0

    1982 doi

  14. [22]

    Monochromatic mass spectrum of primordial black holes

    Kleban, Matthew and Norton, Cameron E. Monochromatic mass spectrum of primordial black holes. Phys. Rev. D. 2025. doi:10.1103/PhysRevD.111.023538. arXiv:2310.09898

    2025 doi

  15. [24]

    , year = 1982, month = jul, volume =

    Electron-Positron Pair Equilibria in Relativistic Plasmas. , year = 1982, month = jul, volume =. doi:10.1086/160082 , adsurl =

    1982 doi

  16. [25]

    , keywords =

    Magnetic Hair and Reconnection in Black Hole Magnetospheres. , keywords =. doi:10.1103/PhysRevLett.127.055101 , archivePrefix =. 2109.14620 , primaryClass =

    doi

  17. [26]

    High resolution schemes for hyperbolic conservation laws , journal =

    Ami Harten , abstract =. High resolution schemes for hyperbolic conservation laws , journal =. 1983 , issn =. doi:https://doi.org/10.1016/0021-9991(83)90136-5 , url =

    1983 doi

  18. [27]

    , keywords =

    Numerical fits to important rates in high temperature astrophysical plasmas. , keywords =. doi:10.1093/mnras/204.4.1269 , adsurl =

    doi

  19. [28]

    Radiative processes in astrophysics

  20. [29]

    Introduction to Stellar Astrophysics

  21. [30]

    , year = 1974, month = aug, volume =

    Black holes in the early Universe. , year = 1974, month = aug, volume =. doi:10.1093/mnras/168.2.399 , adsurl =

    1974 doi

  22. [31]

    , keywords =

    The End of the MACHO Era, Revisited: New Limits on MACHO Masses from Halo Wide Binaries. , keywords =. doi:10.1088/0004-637X/790/2/159 , archivePrefix =. 1406.5169 , primaryClass =

    doi arXiv

  23. [32]

    , keywords =

    Massive black holes in galactic halos ?. , keywords =. doi:10.1086/163729 , adsurl =

    doi

  24. [33]

    , keywords =

    Constraints on MACHO Dark Matter from Compact Stellar Systems in Ultra-faint Dwarf Galaxies. , keywords =. doi:10.3847/2041-8205/824/2/L31 , archivePrefix =. 1605.03665 , primaryClass =

    doi arXiv

  25. [34]

    Black Holes in the Era of Gravitational-Wave Astronomy , year = 2024, editor =

    Primordial black holes. Black Holes in the Era of Gravitational-Wave Astronomy , year = 2024, editor =. doi:10.1016/B978-0-32-395636-9.00012-8 , adsurl =

    2024 doi

  26. [35]

    Classical and Quantum Gravity , keywords =

    Primordial black holes perspectives in gravitational wave astronomy. Classical and Quantum Gravity , keywords =. doi:10.1088/1361-6382/aaa7b4 , archivePrefix =. 1801.05235 , primaryClass =

    doi arXiv

  27. [36]

    , year = 1931, month = jul, volume =

    The Maximum Mass of Ideal White Dwarfs. , year = 1931, month = jul, volume =. doi:10.1086/143324 , adsurl =

    1931 doi

  28. [37]

    , keywords =

    Revisiting constraints on asteroid-mass primordial black holes as dark matter candidates. , keywords =. doi:10.1088/1475-7516/2019/08/031 , archivePrefix =. 1906.05950 , primaryClass =

    2019 doi

  29. [38]

    , keywords =

    Primordial black holes capture by stars and induced collapse to low-mass stellar black holes. , keywords =. doi:10.1093/mnras/stac2647 , archivePrefix =. 2205.13003 , primaryClass =

    doi

  30. [39]

    , keywords =

    Dark matter capture in celestial objects: improved treatment of multiple scattering and updated constraints from white dwarfs. , keywords =. doi:10.1088/1475-7516/2019/08/018 , archivePrefix =. 1906.04204 , primaryClass =

    2019 doi

  31. [40]

    , keywords =

    Dark matter triggers of supernovae. , keywords =. doi:10.1103/PhysRevD.92.063007 , archivePrefix =. 1505.04444 , primaryClass =

    doi arXiv

  32. [41]

    , keywords =

    Primordial black holes captured by neutron stars: Simulations in general relativity. , keywords =. doi:10.1103/PhysRevD.110.023021 , archivePrefix =. 2405.10365 , primaryClass =

    doi

  33. [42]

    , keywords =

    Primordial black holes captured by neutron stars: Relativistic point-mass treatment. , keywords =. doi:10.1103/PhysRevD.109.123012 , archivePrefix =. 2404.08735 , primaryClass =

    doi

  34. [43]

    , keywords =

    Fate of a neutron star with an endoparasitic black hole and implications for dark matter. , keywords =. doi:10.1103/PhysRevD.100.124026 , archivePrefix =. 1909.07968 , primaryClass =

    1909 doi

  35. [44]

    , keywords =

    Accretion onto black holes inside neutron stars with piecewise-polytropic equations of state: Analytic and numerical treatments. , keywords =. doi:10.1103/PhysRevD.104.123021 , archivePrefix =. 2110.08285 , primaryClass =

    doi

  36. [45]

    , keywords =

    Accretion onto a small black hole at the center of a neutron star. , keywords =. doi:10.1103/PhysRevD.103.104009 , archivePrefix =. 2102.09574 , primaryClass =

    doi

  37. [46]

    , keywords =

    Neutron stars harboring a primordial black hole: Maximum survival time. , keywords =. doi:10.1103/PhysRevD.103.L081303 , archivePrefix =. 2101.12220 , primaryClass =

    doi

  38. [47]

    , keywords =

    Growth of black holes in the interior of rotating neutron stars. , keywords =. doi:10.1103/PhysRevD.90.043512 , archivePrefix =. 1312.3764 , primaryClass =

    doi arXiv

  39. [48]

    , keywords =

    Evolution of a primordial black hole inside a rotating solar-type star. , keywords =. doi:10.1093/mnras/277.1.25 , adsurl =

    doi

  40. [49]

    , keywords =

    Mind the Gap: The Location of the Lower Edge of the Pair-instability Supernova Black Hole Mass Gap. , keywords =. doi:10.3847/1538-4357/ab518b , archivePrefix =. 1910.12874 , primaryClass =

    1910 doi

  41. [50]

    , keywords =

    Fragmentation in Gravitationally Unstable Collapsar Disks and Subsolar Neutron Star Mergers. , keywords =. doi:10.3847/2041-8213/ad6990 , archivePrefix =. 2407.07955 , primaryClass =

    doi

  42. [51]

    , keywords =

    Black hole growth through hierarchical black hole mergers in dense star clusters: implications for gravitational wave detections. , keywords =. doi:10.1093/mnras/stz1149 , archivePrefix =. 1811.03640 , primaryClass =

    doi arXiv

  43. [52]

    , keywords =

    Black holes: The next generation repeated mergers in dense star clusters and their gravitational-wave properties. , keywords =. doi:10.1103/PhysRevD.100.043027 , archivePrefix =. 1906.10260 , primaryClass =

    1906 doi

  44. [53]

    , keywords =

    Spinning into the Gap: Direct-horizon Collapse as the Origin of GW231123 from End-to-end General-relativistic Magnetohydrodynamic Simulations. , keywords =. doi:10.3847/2041-8213/ae0d81 , archivePrefix =. 2508.15887 , primaryClass =

    doi

  45. [54]

    , keywords =

    Gravitational waves from primordial black hole mergers. , keywords =. doi:10.1088/1475-7516/2017/09/037 , archivePrefix =. 1707.01480 , primaryClass =

    2017 doi arXiv

  46. [55]

    , keywords =

    Gravitational wave signatures of inflationary models from Primordial Black Hole dark matter. , keywords =. doi:10.1088/1475-7516/2017/09/013 , archivePrefix =. 1707.02441 , primaryClass =

    2017 doi arXiv

  47. [56]

    Physics of the Dark Universe , keywords =

    The clustering of massive Primordial Black Holes as Dark Matter: Measuring their mass distribution with advanced LIGO. Physics of the Dark Universe , keywords =. doi:10.1016/j.dark.2016.10.002 , archivePrefix =. 1603.05234 , primaryClass =

    2016 doi arXiv

  48. [57]

    , keywords =

    Consistency of Primordial Black Hole Dark Matter with LIGO/Virgo Merger Rates. , keywords =. doi:10.1103/PhysRevLett.126.051302 , archivePrefix =. 2007.03565 , primaryClass =

    2007 doi

  49. [58]

    , year = 1971, month = jan, volume =

    Gravitationally collapsed objects of very low mass. , year = 1971, month = jan, volume =. doi:10.1093/mnras/152.1.75 , adsurl =

    1971 doi

  50. [59]

    , keywords =

    Dynamics of Dwarf Galaxies Disfavor Stellar-Mass Black Holes as Dark Matter. , keywords =. doi:10.1103/PhysRevLett.119.041102 , archivePrefix =. 1704.01668 , primaryClass =

    doi arXiv

  51. [60]

    , keywords =

    On the reported death of the MACHO era. , keywords =. doi:10.1111/j.1745-3933.2009.00652.x , archivePrefix =. 0903.1644 , primaryClass =

    2009 doi

  52. [61]

    , keywords =

    The End of the MACHO Era: Limits on Halo Dark Matter from Stellar Halo Wide Binaries. , keywords =. doi:10.1086/380562 , archivePrefix =. astro-ph/0307437 , primaryClass =

    doi arXiv

  53. [62]

    Nature Astronomy , keywords =

    Microlensing constraints on primordial black holes with Subaru/HSC Andromeda observations. Nature Astronomy , keywords =. doi:10.1038/s41550-019-0723-1 , archivePrefix =. 1701.02151 , primaryClass =

    doi arXiv

  54. [63]

    , keywords =

    Constraints on Earth-mass primordial black holes from OGLE 5-year microlensing events. , keywords =. doi:10.1103/PhysRevD.99.083503 , archivePrefix =. 1901.07120 , primaryClass =

    1901 doi arXiv

  55. [64]

    , keywords =

    Microlensing and dynamical constraints on primordial black hole dark matter with an extended mass function. , keywords =. doi:10.1103/PhysRevD.94.063530 , archivePrefix =. 1609.01143 , primaryClass =

    doi arXiv

  56. [65]

    Communications in Mathematical Physics , year = 1975, month = aug, volume =

    Particle creation by black holes. Communications in Mathematical Physics , year = 1975, month = aug, volume =. doi:10.1007/BF02345020 , adsurl =

    1975 doi

  57. [66]

    , keywords =

    Gamma rays from primordial black holes. , keywords =. doi:10.1086/154350 , adsurl =

    doi

  58. [67]

    , keywords =

    New cosmological constraints on primordial black holes. , keywords =. doi:10.1103/PhysRevD.81.104019 , archivePrefix =. 0912.5297 , primaryClass =

    doi arXiv

  59. [68]

    Journal of Physics G Nuclear Physics , keywords =

    Primordial black holes as a dark matter candidate. Journal of Physics G Nuclear Physics , keywords =. doi:10.1088/1361-6471/abc534 , archivePrefix =. 2007.10722 , primaryClass =

    2007 doi arXiv

  60. [69]

    , keywords =

    Inflation and primordial black holes as dark matter. , keywords =. doi:10.1103/PhysRevD.50.7173 , adsurl =

    doi

  61. [70]

    , keywords =

    Massive primordial black holes from hybrid inflation as dark matter and the seeds of galaxies. , keywords =. doi:10.1103/PhysRevD.92.023524 , archivePrefix =. 1501.07565 , primaryClass =

    doi arXiv

  62. [71]

    Annual Review of Nuclear and Particle Science , keywords =

    Primordial Black Holes as Dark Matter: Recent Developments. Annual Review of Nuclear and Particle Science , keywords =. doi:10.1146/annurev-nucl-050520-125911 , archivePrefix =. 2006.02838 , primaryClass =

    2006 doi arXiv

  63. [72]

    Annalen der Physik , keywords =

    Peculiar relics from Primordial Black Holes in the inflationary paradigm. Annalen der Physik , keywords =. doi:10.1002/andp.200310067 , archivePrefix =. astro-ph/0303330 , primaryClass =

    doi arXiv

  64. [73]

    , keywords =

    The primordial black hole mass spectrum. , keywords =. doi:10.1086/153853 , adsurl =

    doi

  65. [74]

    Reports on Progress in Physics , keywords =

    Constraints on primordial black holes. Reports on Progress in Physics , keywords =. doi:10.1088/1361-6633/ac1e31 , archivePrefix =. 2002.12778 , primaryClass =

    2002 doi arXiv

  66. [75]

    , keywords =

    Primordial black holes as dark matter. , keywords =. doi:10.1103/PhysRevD.94.083504 , archivePrefix =. 1607.06077 , primaryClass =

    doi arXiv

  67. [76]

    , year = 1999, month = aug, volume =

    A compilation of charged-particle induced thermonuclear reaction rates. , year = 1999, month = aug, volume =. doi:10.1016/S0375-9474(99)00030-5 , adsurl =

    1999 doi

  68. [77]

    1969 , institution =

    1969

  69. [78]

    , keywords =

    Rosseland and Flux Mean Opacities for Compton Scattering. , keywords =. doi:10.3847/1538-4357/835/2/119 , archivePrefix =. 1606.09466 , primaryClass =

    doi arXiv

  70. [79]

    arXiv e-prints , keywords =

    High Metal Content of Highly Accreting Quasars: Analysis of an Extended Sample. arXiv e-prints , keywords =

  71. [80]

    Journal of High Energy Physics , keywords =

    Orbital dynamics of the solar basin. Journal of High Energy Physics , keywords =. doi:10.1007/JHEP12(2024)007 , archivePrefix =. 2408.16041 , primaryClass =

    2024 doi

  72. [81]

    doi:10.1007/978-3-642-30304-3 , adsurl =

    Stellar Structure and Evolution. doi:10.1007/978-3-642-30304-3 , adsurl =

    doi

  73. [82]

    and Haberland, Matt and Reddy, Tyler and Cournapeau, David and Burovski, Evgeni and Peterson, Pearu and Weckesser, Warren and Bright, Jonathan and

    Virtanen, Pauli and Gommers, Ralf and Oliphant, Travis E. and Haberland, Matt and Reddy, Tyler and Cournapeau, David and Burovski, Evgeni and Peterson, Pearu and Weckesser, Warren and Bright, Jonathan and. Nature Methods , year =

  74. [83]

    American journal of Mathematics , volume=

    Researches in the lunar theory , author=. American journal of Mathematics , volume=. 1878 , publisher=

  75. [84]

    , title =

    Podsiadlowski,Philipp and Rees,Martin J. , title =. AIP Conference Proceedings , volume =. 1994 , doi =

    1994

  76. [85]

    , year = 1952, month = jan, volume =

    On spherically symmetrical accretion. , year = 1952, month = jan, volume =. doi:10.1093/mnras/112.2.195 , adsurl =

    1952 doi

  77. [86]

    , keywords =

    Making massive stars in the Galactic Centre via accretion on to low-mass stars within an accretion disc. , keywords =. doi:10.1093/mnras/staa2590 , archivePrefix =. 2008.10033 , primaryClass =

    2008 doi

  78. [87]

    The Multi-Messenger Astrophysics of the Galactic Centre , year = 2017, editor =

    Observational constraints on the formation and evolution of the Milky Way nuclear star cluster with Keck and Gemini. The Multi-Messenger Astrophysics of the Galactic Centre , year = 2017, editor =. doi:10.1017/S1743921316012230 , archivePrefix =. 1610.02964 , primaryClass =

    2017 doi arXiv

  79. [88]

    , keywords =

    A model for time-dependent turbulent convection. , keywords =

  80. [89]

    , keywords =

    Rapid Black Hole Spin-down by Thick Magnetically Arrested Disks. , keywords =. doi:10.3847/1538-4357/ad09af , archivePrefix =. 2302.01351 , primaryClass =

    doi

  81. [90]

    , keywords =

    She's Got Her Mother's Hair: Unveiling the Origin of Black Hole Magnetic Fields through Stellar to Collapsar Simulations. , keywords =. doi:10.3847/2041-8213/ad8563 , archivePrefix =. 2407.16745 , primaryClass =

    doi

  82. [91]

    , keywords =

    Dynamo action by differential rotation in a stably stratified stellar interior. , keywords =. doi:10.1051/0004-6361:20011465 , archivePrefix =. astro-ph/0108207 , primaryClass =

    doi arXiv

  83. [92]

    , keywords =

    Slowing the spins of stellar cores. , keywords =. doi:10.1093/mnras/stz514 , archivePrefix =. 1902.08227 , primaryClass =

    1902 doi arXiv

  84. [93]

    arXiv e-prints , keywords =

    Tayler Instability Revisited. arXiv e-prints , keywords =. doi:10.48550/arXiv.2404.19103 , archivePrefix =. 2404.19103 , primaryClass =

    doi

  85. [94]

    , keywords =

    Large scale magnetic fields and their dissipation in GRB fireballs\. , keywords =. doi:10.1051/0004-6361:20010131 , archivePrefix =. astro-ph/0004274 , primaryClass =

    doi arXiv

  86. [95]

    , year = 1973, month = jan, volume =

    The adiabatic stability of stars containing magnetic fields-I.Toroidal fields. , year = 1973, month = jan, volume =. doi:10.1093/mnras/161.4.365 , adsurl =

    1973 doi

  87. [96]

    , keywords =

    Collapsar Gamma-Ray Bursts Grind Their Black Hole Spins to a Halt. , keywords =. doi:10.3847/1538-4357/ad02f0 , archivePrefix =. 2302.07281 , primaryClass =

    doi

  88. [97]

    , keywords =

    H-AMR: A New GPU-accelerated GRMHD Code for Exascale Computing with 3D Adaptive Mesh Refinement and Local Adaptive Time Stepping. , keywords =. doi:10.3847/1538-4365/ac9966 , archivePrefix =. 1912.10192 , primaryClass =

    1912 doi

  89. [98]

    , year = 1970, month = apr, volume =

    Kerr Metric Black Holes. , year = 1970, month = apr, volume =. doi:10.1038/226064a0 , adsurl =

    1970 doi

  90. [99]

    , keywords =

    Solar Evolution Models with a Central Black Hole. , keywords =. doi:10.3847/1538-4357/ad04de , archivePrefix =. 2312.06782 , primaryClass =

    doi

  91. [100]

    , keywords =

    Is there a black hole in the center of the Sun?. , keywords =. doi:10.1007/s10509-024-04270-1 , archivePrefix =. 2312.07647 , primaryClass =

    doi

  92. [101]

    , keywords =

    Modules for Experiments in Stellar Astrophysics (MESA): Time-dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure. , keywords =. doi:10.3847/1538-4365/acae8d , archivePrefix =. 2208.03651 , primaryClass =

    doi

  93. [102]

    , keywords =

    The Stellar Cusp around the Supermassive Black Hole in the Galactic Center. , keywords =. 2003. doi:10.1086/377127 , archivePrefix =. astro-ph/0305423 , primaryClass =

    2003 doi arXiv

  94. [103]

    , keywords =

    The Stellar Merger Scenario for Black Holes in the Pair-instability Gap. , keywords =. doi:10.3847/2041-8213/abc6a6 , archivePrefix =. 2010.00705 , primaryClass =

    doi

  95. [104]

    , keywords =

    High Angular Resolution Integral-Field Spectroscopy of the Galaxy's Nuclear Cluster: A Missing Stellar Cusp?. , keywords =. 2009. doi:10.1088/0004-637X/703/2/1323 , archivePrefix =. 0908.0311 , primaryClass =

    2009 doi arXiv

  96. [105]

    , keywords =

    Stellar Dynamics and Stellar Phenomena Near a Massive Black Hole. , keywords =. 2017. doi:10.1146/annurev-astro-091916-055306 , archivePrefix =. 1701.04762 , primaryClass =

    2017 doi arXiv

  97. [106]

    Introduction to Stellar Winds

  98. [108]

    , keywords =

    Revisiting the Unified Model of Active Galactic Nuclei. , keywords =. 2015. doi:10.1146/annurev-astro-082214-122302 , archivePrefix =. 1505.00811 , primaryClass =

    2015 doi arXiv

  99. [109]

    , keywords =

    Starbursts near supermassive black holes: young stars in the Galactic Centre, and gravitational waves in LISA band. , keywords =. doi:10.1111/j.1365-2966.2006.11155.x , archivePrefix =. astro-ph/0603583 , primaryClass =

    2006 doi

  100. [110]

    , keywords =

    Stellar Disk in the Galactic Center: A Remnant of a Dense Accretion Disk?. , keywords =. doi:10.1086/376675 , archivePrefix =. astro-ph/0303436 , primaryClass =

    doi arXiv

  101. [111]

    , keywords =

    An Extremely Top-Heavy Initial Mass Function in the Galactic Center Stellar Disks. , keywords =. 2010. doi:10.1088/0004-637X/708/1/834 , archivePrefix =. 0908.2177 , primaryClass =

    2010 doi arXiv

  102. [112]

    , keywords =

    The First Measurement of Spectral Lines in a Short-Period Star Bound to the Galaxy's Central Black Hole: A Paradox of Youth. , keywords =. 2003. doi:10.1086/374804 , archivePrefix =. astro-ph/0302299 , primaryClass =

    2003 doi arXiv

  103. [113]

    , keywords =

    Star distribution around a massive black hole in a globular cluster. , keywords =. doi:10.1086/154711 , adsurl =

    doi

  104. [114]

    , keywords =

    The Two Young Star Disks in the Central Parsec of the Galaxy: Properties, Dynamics, and Formation. , keywords =. doi:10.1086/503273 , archivePrefix =. astro-ph/0601268 , primaryClass =

    doi arXiv

  105. [115]

    The star distribution around a massive black hole in a globular cluster. II. Unequal star masses. , keywords =. doi:10.1086/155534 , adsurl =

    doi

  106. [116]

    , keywords =

    On the Nature of the Fast-Moving Star S2 in the Galactic Center. , keywords =. doi:10.1086/526768 , archivePrefix =. 0711.3344 , primaryClass =

    doi arXiv

  107. [117]

    , keywords =

    Super-solar Metallicity Stars in the Galactic Center Nuclear Star Cluster: Unusual Sc, V, and Y Abundances. , keywords =. doi:10.3847/2041-8213/aaaec3 , archivePrefix =. 1802.08270 , primaryClass =

    doi arXiv

  108. [118]

    2006 , Bdsk-Url-1 =

    Daramy-Loirat, Catherine and Defour, David and de Dinechin, Florent and Gallet, Matthieu and Gast, Nicolas and Lauter, Christoph and Muller, Jean-Michel , hal_id =. 2006 , Bdsk-Url-1 =

    2006

  109. [119]

    , year = 1929, month = nov, volume =

    Internal circulation in rotating stars. , year = 1929, month = nov, volume =. doi:10.1093/mnras/90.1.54 , adsurl =

    1929 doi

  110. [120]

    arXiv e-prints , keywords =

    Three Dimensional Radiation Hydrodynamic Simulations of Massive Star Envelopes. arXiv e-prints , keywords =

  111. [121]

    , keywords =

    Accretion-modified Stars in Accretion Disks of Active Galactic Nuclei: Slowly Transient Appearance. , keywords =. doi:10.3847/2041-8213/abee81 , archivePrefix =. 2103.07708 , primaryClass =

    doi

  112. [122]

    , keywords =

    Accretion onto Stars in the Disks of Active Galactic Nuclei. , keywords =. doi:10.3847/1538-4357/ac042c , archivePrefix =. 2102.12484 , primaryClass =

    doi

  113. [123]

    , journal =

    Kutta, W. , journal =. Beitrag zur n\"aherungsweisen

  114. [124]

    Proceedings of the Cambridge Philosophical Society , year = 1939, month = jan, volume =

    The effect of interstellar matter on climatic variation. Proceedings of the Cambridge Philosophical Society , year = 1939, month = jan, volume =. doi:10.1017/S0305004100021150 , adsurl =

    1939 doi

  115. [125]

    , keywords =

    Hydrodynamic calculations of axisymmetric accretion flow. , keywords =. doi:10.1093/mnras/217.2.367 , adsurl =

    doi

  116. [126]

    , keywords =

    Stellar Evolution in AGN Disks. , keywords =. doi:10.3847/1538-4357/abdf4f , archivePrefix =. 2009.03936 , primaryClass =

    2009 doi

  117. [127]

    , keywords =

    Star formation in accretion discs and SMBH growth. , keywords =. doi:10.1093/mnras/staa463 , archivePrefix =. 1911.08685 , primaryClass =

    1911 doi

  118. [128]

    , keywords =

    Bondi Accretion in the Presence of Vorticity. , keywords =. doi:10.1086/426051 , archivePrefix =. astro-ph/0409454 , primaryClass =

    doi arXiv

  119. [129]

    , keywords =

    How consumption and repulsion set planetary gap depths and the final masses of gas giants. , keywords =. doi:10.1093/mnras/staa1721 , archivePrefix =. 2004.13720 , primaryClass =

    2004 doi

  120. [130]

    , keywords =

    Deep and wide gaps by super Earths in low-viscosity discs. , keywords =. doi:10.1093/mnras/sty1466 , archivePrefix =. 1803.01868 , primaryClass =

    doi arXiv

  121. [131]

    , keywords =

    Tidal Barrier and the Asymptotic Mass of Proto-Gas Giant Planets. , keywords =. doi:10.1086/512537 , archivePrefix =. astro-ph/0701269 , primaryClass =

    doi arXiv

  122. [132]

    , keywords =

    Nuclear star clusters. , keywords =. doi:10.1007/s00159-020-00125-0 , archivePrefix =. 2001.03626 , primaryClass =

    2001 doi

  123. [133]

    , keywords =

    Observational constraints on growth of massive black holes. , keywords =. doi:10.1046/j.1365-8711.2002.05532.x , archivePrefix =. astro-ph/0203082 , primaryClass =

    2002 doi

  124. [134]

    , keywords =

    Masses of quasars. , keywords =. doi:10.1093/mnras/200.1.115 , adsurl =

    doi

  125. [135]

    , keywords =

    Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies. , keywords =. doi:10.1146/annurev-astro-082708-101811 , archivePrefix =. 1304.7762 , primaryClass =

    doi arXiv

  126. [136]

    , year = 1969, month = aug, volume =

    Galactic Nuclei as Collapsed Old Quasars. , year = 1969, month = aug, volume =. doi:10.1038/223690a0 , adsurl =

    1969 doi

  127. [137]

    , keywords =

    Nuclear activity in nearby galaxies. , keywords =. doi:10.1146/annurev.astro.45.051806.110546 , archivePrefix =. 0803.2268 , primaryClass =

    doi arXiv

  128. [139]

    , keywords =

    Active galactic nuclei flicker: an observational estimate of the duration of black hole growth phases of 10 ^ 5 yr. , keywords =. doi:10.1093/mnras/stv1136 , archivePrefix =. 1505.06733 , primaryClass =

    doi arXiv

  129. [140]

    , keywords =

    Star Trapping and Metallicity Enrichment in Quasars and Active Galactic Nuclei. , keywords =. doi:10.1086/172690 , adsurl =

    doi

  130. [141]

    , keywords =

    The Effect of Star-Disk Interactions on Highly Eccentric Stellar Orbits in Active Galactic Nuclei: A Disk Loss Cone and Implications for Stellar Tidal Disruption Events. , keywords =. doi:10.3847/1538-4357/ab64db , archivePrefix =. 1909.09645 , primaryClass =

    1909 doi

  131. [142]

    , keywords =

    Dynamical evolution of star clusters around a rotating black hole with an accretion disc. , keywords =. doi:10.1093/mnras/275.3.628 , adsurl =

    doi

  132. [143]

    Three-dimensional Interaction between a Planet and an Isothermal Gaseous Disk. II. Eccentricity Waves and Bending Waves. , keywords =. doi:10.1086/380992 , adsurl =

    doi

  133. [144]

    , year = 1964, month = may, volume =

    On the gravitational stability of a disk of stars. , year = 1964, month = may, volume =. doi:10.1086/147861 , adsurl =

    1964 doi

  134. [145]

    , keywords =

    Nonlinear Outcome of Gravitational Instability in Cooling, Gaseous Disks. , keywords =. doi:10.1086/320631 , archivePrefix =. astro-ph/0101501 , primaryClass =

    doi arXiv

  135. [146]

    , keywords =

    Gas metallicity diagnostics in star-forming galaxies. , keywords =. doi:10.1051/0004-6361:20065216 , archivePrefix =. astro-ph/0603580 , primaryClass =

    doi arXiv

  136. [147]

    , keywords =

    The evolution of chemical abundance in quasar broad line region. , keywords =. doi:10.1093/mnras/sty1763 , archivePrefix =. 1807.01978 , primaryClass =

    doi arXiv

  137. [148]

    , keywords =

    Aligning Nuclear Cluster Orbits with an Active Galactic Nucleus Accretion Disc. , keywords =. doi:10.1093/mnras/staa3004 , archivePrefix =. 2006.11229 , primaryClass =

    2006 doi

  138. [149]

    , year = 1995, month = jun, volume =

    Gravitationally redshifted emission implying an accretion disk and massive black hole in the active galaxy MCG-6-30-15. , year = 1995, month = jun, volume =. doi:10.1038/375659a0 , adsurl =

    1995 doi

  139. [150]

    , keywords =

    On the Dependence of the Iron K-Line Profiles with Luminosity in Active Galactic Nuclei. , keywords =. doi:10.1086/310937 , archivePrefix =. astro-ph/9708030 , primaryClass =

    doi arXiv

  140. [151]

    , keywords =

    Alternative Explanations for Extreme Supersolar Iron Abundances Inferred from the Energy Spectrum of Cygnus X-1. , keywords =. doi:10.3847/1538-4357/aaaab1 , archivePrefix =. 1801.07267 , primaryClass =

    doi arXiv

  141. [152]

    Workshop on Astrophysical Opacities , year = 2018, series =

    The Problem of the High Iron Abundance in Accretion Disks around Black Holes. Workshop on Astrophysical Opacities , year = 2018, series =

    2018

  142. [153]

    arXiv e-prints , keywords =

    FORGE'd in FIRE III: The IMF in Quasar Accretion Disks from STARFORGE. arXiv e-prints , keywords =. doi:10.48550/arXiv.2404.08046 , archivePrefix =. 2404.08046 , primaryClass =

    doi

  143. [154]

    Black holes in binary systems

    Reprint of 1973A&A....24..337S. Black holes in binary systems. Observational appearance. , year = 1973, month = jun, volume =

    1973

  144. [155]

    , keywords =

    Formation of primordial supermassive stars by burst accretion. , keywords =. doi:10.1093/mnras/stv1346 , archivePrefix =. 1505.03954 , primaryClass =

    doi arXiv

  145. [156]

    , keywords =

    The Influence of Disk Composition on the Evolution of Stars in the Disks of Active Galactic Nuclei. , keywords =. doi:10.3847/1538-4357/acacf2 , archivePrefix =. 2209.05499 , primaryClass =

    doi

  146. [157]

    , keywords =

    Accretion disc viscosity: how big is alpha?. , keywords =. doi:10.1111/j.1365-2966.2007.11556.x , archivePrefix =. astro-ph/0701803 , primaryClass =

    2007 doi

  147. [158]

    Black Holes (Les Astres Occlus) , year = 1973, month = jan, pages =

    Astrophysics of black holes. Black Holes (Les Astres Occlus) , year = 1973, month = jan, pages =

    1973

  148. [159]

    , keywords =

    A theory of the instability of disk accretion on to black holes and the variability of binary X-ray sources, galactic nuclei and quasars. , keywords =. doi:10.1093/mnras/175.3.613 , adsurl =

    doi

  149. [160]

    , keywords =

    Opacity-driven Convection and Variability in Accretion Disks around Supermassive Black Holes. , keywords =. doi:10.3847/1538-4357/aba4b7 , archivePrefix =. 2006.08657 , primaryClass =

    2006 doi

  150. [161]

    , keywords =

    Super-Eddington Accretion Disks around Supermassive Black Holes. , keywords =. doi:10.3847/1538-4357/ab29ff , archivePrefix =. 1709.02845 , primaryClass =

    doi

  151. [162]

    , keywords =

    Global Radiation Magnetohydrodynamic Simulations of sub-Eddington Accretion Disks around Supermassive Black Holes. , keywords =. doi:10.3847/1538-4357/ab4a00 , archivePrefix =. 1904.01674 , primaryClass =

    1904 doi

  152. [163]

    Active Galactic Nuclei , year = 1990, editor =

    AGN emission lines. Active Galactic Nuclei , year = 1990, editor =

    1990

  153. [164]

    , keywords =

    Feedback-dominated Accretion Flows. , keywords =. doi:10.3847/1538-4357/ac4ded , archivePrefix =. 2107.07519 , primaryClass =

    doi

  154. [165]

    arXiv e-prints , keywords =

    Time-dependent models of AGN disks with radiation from embedded stellar-mass black holes. arXiv e-prints , keywords =. doi:10.48550/arXiv.2405.09380 , archivePrefix =. 2405.09380 , primaryClass =

    doi

  155. [166]

    , keywords =

    Spectral energy distributions of marginally self-gravitating quasi-stellar object discs. , keywords =. doi:10.1046/j.1365-8711.2003.06431.x , archivePrefix =. astro-ph/0209469 , primaryClass =

    2003 doi

  156. [167]

    , keywords =

    Stellar Black Holes Can ``Stretch'' Supermassive Black Hole Accretion Disks. , keywords =. doi:10.3847/2041-8213/ad3c3f , archivePrefix =. 2404.07407 , primaryClass =

    doi

  157. [168]

    , keywords =

    Radiation Pressure-supported Starburst Disks and Active Galactic Nucleus Fueling. , keywords =. doi:10.1086/431923 , archivePrefix =. astro-ph/0503027 , primaryClass =

    doi arXiv

  158. [169]

    , keywords =

    Time development of the emission lines and continuum of NGC 4151. , keywords =. doi:10.1086/161223 , adsurl =

    doi

  159. [170]

    , keywords =

    Are the Variations in Quasar Optical Flux Driven by Thermal Fluctuations?. , keywords =. doi:10.1088/0004-637X/698/1/895 , archivePrefix =. 0903.5315 , primaryClass =

    doi arXiv

  160. [171]

    , keywords =

    Modeling the Time Variability of SDSS Stripe 82 Quasars as a Damped Random Walk. , keywords =. doi:10.1088/0004-637X/721/2/1014 , archivePrefix =. 1004.0276 , primaryClass =

    doi arXiv

  161. [172]

    , keywords =

    Boundary Layer Circumplanetary Accretion: How Fast Could an Unmagnetized Planet Spin Up through Its Disk?. , keywords =. doi:10.3847/1538-4357/ac1941 , archivePrefix =. 2012.06641 , primaryClass =

    2012 doi

  162. [173]

    , keywords =

    Quasar Accretion Disks are Strongly Inhomogeneous. , keywords =. doi:10.1088/2041-8205/727/1/L24 , archivePrefix =. 1012.3169 , primaryClass =

    doi arXiv

  163. [174]

    , year = 1997, month = apr, volume =

    Protoplanet Migration by Nebula Tides. , year = 1997, month = apr, volume =. doi:10.1006/icar.1996.5647 , adsurl =

    1997 doi

  164. [175]

    X-Ray and Optical Flux Ratio Anomalies in Quadruply Lensed Quasars. I. Zooming in on Quasar Emission Regions. , keywords =. doi:10.1086/512115 , archivePrefix =. astro-ph/0607655 , primaryClass =

    doi arXiv

  165. [176]

    , keywords =

    The Sizes of the X-ray and Optical Emission Regions of RXJ 1131-1231. , keywords =. doi:10.1088/0004-637X/709/1/278 , archivePrefix =. 0906.4342 , primaryClass =

    doi arXiv

  166. [177]

    , keywords =

    The Quasar Accretion Disk Size-Black Hole Mass Relation. , keywords =. doi:10.1088/0004-637X/712/2/1129 , archivePrefix =. 1002.4160 , primaryClass =

    doi arXiv

  167. [178]

    , keywords =

    The Effect of a Time-varying Accretion Disk Size on Quasar Microlensing Light Curves. , keywords =. doi:10.1088/0004-637X/718/2/1079 , archivePrefix =. 1002.3126 , primaryClass =

    doi arXiv

  168. [179]

    , keywords =

    The Discovery of the First Changing Look Quasar: New Insights Into the Physics and Phenomenology of Active Galactic Nucleus. , keywords =. doi:10.1088/0004-637X/800/2/144 , archivePrefix =. 1412.2136 , primaryClass =

    doi arXiv

  169. [180]

    , keywords =

    Changing-look Quasar Candidates: First Results from Follow-up Spectroscopy of Highly Optically Variable Quasars. , keywords =. doi:10.3847/1538-4357/ab05e2 , archivePrefix =. 1810.00087 , primaryClass =

    doi arXiv

  170. [181]

    , keywords =

    A New Class of Changing-look LINERs. , keywords =. doi:10.3847/1538-4357/ab3a38 , archivePrefix =. 1904.10973 , primaryClass =

    1904 doi

  171. [182]

    , keywords =

    Assisted inspirals of stellar mass black holes embedded in AGN discs: solving the `final au problem'. , keywords =. doi:10.1093/mnras/stw2260 , archivePrefix =. 1602.04226 , primaryClass =

    doi arXiv

  172. [183]

    , keywords =

    Constraining Stellar-mass Black Hole Mergers in AGN Disks Detectable with LIGO. , keywords =. doi:10.3847/1538-4357/aadae5 , archivePrefix =. 1702.07818 , primaryClass =

    doi arXiv

  173. [184]

    , keywords =

    Stellar processes near the massive black hole in the Galactic center [review article]. , keywords =. 2005. doi:10.1016/j.physrep.2005.08.002 , archivePrefix =. astro-ph/0508106 , primaryClass =

    2005 doi arXiv

  174. [185]

    , keywords =

    Stellar and wind properties of massive stars in the central parsec of the Galaxy. , keywords =. doi:10.1051/0004-6361:20066688 , archivePrefix =. astro-ph/0703211 , primaryClass =

    doi arXiv

  175. [186]

    , keywords =

    Giant Gamma-ray Bubbles from Fermi-LAT: Active Galactic Nucleus Activity or Bipolar Galactic Wind?. , keywords =. doi:10.1088/0004-637X/724/2/1044 , archivePrefix =. 1005.5480 , primaryClass =

    doi arXiv

  176. [187]

    , keywords =

    The Large-scale Ionization Cones in the Galaxy. , keywords =. doi:10.3847/1538-4357/ab44c8 , archivePrefix =. 1910.02225 , primaryClass =

    1910 doi

  177. [188]

    , keywords =

    Twelve Years of Spectroscopic Monitoring in the Galactic Center: The Closest Look at S-stars near the Black Hole. , keywords =. doi:10.3847/1538-4357/aa876f , archivePrefix =. 1708.06353 , primaryClass =

    doi arXiv

  178. [189]

    , keywords =

    Black hole, neutron star, and white dwarf merger rates in AGN discs. , keywords =. doi:10.1093/mnras/staa2681 , archivePrefix =. 2002.00046 , primaryClass =

    2002 doi

  179. [190]

    Reviews of Modern Physics , keywords =

    The Galactic Center massive black hole and nuclear star cluster. Reviews of Modern Physics , keywords =. doi:10.1103/RevModPhys.82.3121 , archivePrefix =. 1006.0064 , primaryClass =

    doi arXiv

  180. [191]

    , year = 2018, month = apr, volume =

    A density cusp of quiescent X-ray binaries in the central parsec of the Galaxy. , year = 2018, month = apr, volume =. doi:10.1038/nature25029 , adsurl =

    2018 doi

  181. [192]

    On the Tidal Interaction between Protoplanets and the Protoplanetary Disk. III. Orbital Migration of Protoplanets. , keywords =. doi:10.1086/164653 , adsurl =

    doi

  182. [193]

    Physical Review , year = 1939, month = mar, volume =

    Energy Production in Stars. Physical Review , year = 1939, month = mar, volume =. doi:10.1103/PhysRev.55.434 , adsurl =

    1939 doi

  183. [194]

    , keywords =

    Formation and Evolution of Compact-object Binaries in AGN Disks. , keywords =. doi:10.3847/1538-4357/ab9b8c , archivePrefix =. 1912.08218 , primaryClass =

    1912 doi

  184. [195]

    , keywords =

    Stellar Neutrino Emission across the Mass-Metallicity Plane. , keywords =. doi:10.3847/1538-4365/ad0787 , archivePrefix =. 2310.13142 , primaryClass =

    doi

  185. [196]

    , keywords =

    Probing gas disc physics with LISA: simulations of an intermediate mass ratio inspiral in an accretion disc. , keywords =. doi:10.1093/mnras/stz1026 , archivePrefix =. 1810.03623 , primaryClass =

    doi

  186. [197]

    , keywords =

    The Migration of Gap-opening Planets is Not Locked to Viscous Disk Evolution. , keywords =. doi:10.1088/2041-8205/792/1/L10 , archivePrefix =. 1405.3711 , primaryClass =

    doi arXiv

  187. [198]

    , keywords =

    Evolution of gas disc-embedded intermediate mass ratio inspirals in the LISA band. , keywords =. doi:10.1093/mnras/staa3976 , archivePrefix =. 2005.11333 , primaryClass =

    2005 doi

  188. [199]

    , keywords =

    Extreme Variability Quasars from the Sloan Digital Sky Survey and the Dark Energy Survey. , keywords =. doi:10.3847/1538-4357/aaa9b6 , archivePrefix =. 1706.07875 , primaryClass =

    doi arXiv

  189. [200]

    , keywords =

    The evolution of irradiated stars. , keywords =. doi:10.1093/mnras/238.2.427 , adsurl =

    doi

  190. [201]

    , keywords =

    Pileups and Migration Rates for Planets in Low-mass Disks. , keywords =. doi:10.3847/1538-4357/ab723c , archivePrefix =. 1908.02326 , primaryClass =

    1908 doi

  191. [202]

    SIRIUS project. III. Star-by-star simulations of star cluster formation using a direct N-body integrator with stellar feedback. , keywords =. doi:10.1093/pasj/psab061 , archivePrefix =. 2103.02829 , primaryClass =

    doi

  192. [203]

    Evolution of single and binary compact objects in star clusters with up to 1 million stars

    The DRAGON-II simulations - I. Evolution of single and binary compact objects in star clusters with up to 1 million stars. , keywords =. doi:10.1093/mnras/stad3952 , archivePrefix =. 2307.04805 , primaryClass =

    doi

  193. [204]

    , keywords =

    The Population of Massive Stars in Active Galactic Nuclei Disks. , keywords =. doi:10.3847/1538-4357/ad3c3a , archivePrefix =. 2404.08780 , primaryClass =

    doi

  194. [205]

    , keywords =

    Was the nineteenth century giant eruption of Eta Carinae a merger event in a triple system?. , keywords =. doi:10.1093/mnras/stv2787 , archivePrefix =. 1511.06889 , primaryClass =

    doi arXiv

  195. [206]

    , keywords =

    Simulations of the tidal interaction and mass transfer of a star in an eccentric orbit around an intermediate-mass black hole: the case of HLX-1. , keywords =. doi:10.1093/mnras/stv2318 , archivePrefix =. 1510.01879 , primaryClass =

    doi arXiv

  196. [207]

    , keywords =

    Accretion rates of protoplanets. , keywords =. doi:10.1016/0019-1035(90)90021-Z , adsurl =

    doi

  197. [208]

    , keywords =

    A two-temperature accretion disk model for Cygnus X-1: structure and spectrum. , keywords =. doi:10.1086/154162 , adsurl =

    doi

  198. [209]

    , keywords =

    The impermanent fate of massive stars in AGN discs. , keywords =. doi:10.1093/mnras/stad2774 , archivePrefix =. 2309.04392 , primaryClass =

    doi

  199. [210]

    , keywords =

    Accretion of Gas Giants Constrained by the Tidal Barrier. , keywords =. doi:10.3847/1538-4357/abc883 , archivePrefix =. 2011.02869 , primaryClass =

    2011 doi

  200. [211]

    , keywords =

    Supermassive Stars in Quasar Disks. , keywords =. doi:10.1086/386360 , archivePrefix =. astro-ph/0307361 , primaryClass =

    doi arXiv

  201. [212]

    , keywords =

    Modelling of deep gaps created by giant planets in protoplanetary disks. , keywords =. doi:10.1093/pasj/psx114 , archivePrefix =. 1609.02706 , primaryClass =

    doi arXiv

  202. [213]

    Radial Migration of Gap-opening Planets in Protoplanetary Disks. I. The Case of a Single Planet. , keywords =. doi:10.3847/1538-4357/aac8d9 , archivePrefix =. 1805.11101 , primaryClass =

    doi arXiv

  203. [214]

    , keywords =

    Migration of massive planets in accreting disks. , keywords =. doi:10.1051/0004-6361/201424837 , archivePrefix =. 1411.3190 , primaryClass =

    doi arXiv

  204. [215]

    , keywords =

    A Porosity-Length Formalism for Photon-Tiring-limited Mass Loss from Stars above the Eddington Limit. , keywords =. doi:10.1086/424910 , archivePrefix =. astro-ph/0409573 , primaryClass =

    doi arXiv

  205. [216]

    , keywords =

    Mass Loss: Its Effect on the Evolution and Fate of High-Mass Stars. , keywords =. doi:10.1146/annurev-astro-081913-040025 , archivePrefix =. 1402.1237 , primaryClass =

    doi arXiv

  206. [217]

    , keywords =

    A Simple Analytical Model for Gaps in Protoplanetary Disks. , keywords =. doi:10.1088/2041-8205/807/1/L11 , archivePrefix =. 1505.03514 , primaryClass =

    doi arXiv

  207. [218]

    , keywords =

    Testing the Propagating Fluctuations Model with a Long, Global Accretion Disk Simulation. , keywords =. doi:10.3847/0004-637X/826/1/40 , archivePrefix =. 1512.05350 , primaryClass =

    doi arXiv

  208. [219]

    , keywords =

    Gap Opening by Extremely Low-mass Planets in a Viscous Disk. , keywords =. doi:10.1088/0004-637X/769/1/41 , archivePrefix =. 1302.1934 , primaryClass =

    1934 doi arXiv

  209. [220]

    , keywords =

    The Vertical Structure and Stability of Accretion Disks Surrounding Black Holes and Neutron Stars. , keywords =. doi:10.1086/173680 , adsurl =

    doi

  210. [221]

    , keywords =

    Gravity darkening in rotating stars. , keywords =. doi:10.1051/0004-6361/201117252 , archivePrefix =. 1109.3038 , primaryClass =

    doi arXiv

  211. [222]

    , keywords =

    Vertical structure of accretion disks. , keywords =

  212. [223]

    doi:10.1007/978-3-540-76949-1 , adsurl =

    Physics, Formation and Evolution of Rotating Stars. doi:10.1007/978-3-540-76949-1 , adsurl =

    doi

  213. [224]

    , keywords =

    Massive main-sequence stars evolving at the Eddington limit. , keywords =. doi:10.1051/0004-6361/201525945 , archivePrefix =. 1506.02997 , primaryClass =

    doi arXiv

  214. [225]

    , keywords =

    Modules for Experiments in Stellar Astrophysics (MESA). , keywords =. doi:10.1088/0067-0049/192/1/3 , archivePrefix =. 1009.1622 , primaryClass =

    doi arXiv

  215. [226]

    , keywords =

    Models of Radiation-driven Winds from General Relativistic Neutron Stars. , keywords =. doi:10.1086/164012 , adsurl =

    doi

  216. [227]

    , keywords =

    Modules for Experiments in Stellar Astrophysics (MESA): Planets, Oscillations, Rotation, and Massive Stars. , keywords =. doi:10.1088/0067-0049/208/1/4 , archivePrefix =. 1301.0319 , primaryClass =

    doi arXiv

  217. [228]

    , keywords =

    Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions. , keywords =. doi:10.1088/0067-0049/220/1/15 , archivePrefix =. 1506.03146 , primaryClass =

    doi arXiv

  218. [229]

    , keywords =

    Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions. , keywords =. doi:10.3847/1538-4365/aaa5a8 , archivePrefix =. 1710.08424 , primaryClass =

    doi arXiv

  219. [230]

    , keywords =

    Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation. , keywords =. doi:10.3847/1538-4365/ab2241 , archivePrefix =. 1903.01426 , primaryClass =

    1903 doi arXiv

  220. [231]

    The Mathematica Journal , year = 2014, volume =

    On B. The Mathematica Journal , year = 2014, volume =

    2014

  221. [232]

    A course of modern analysis

  222. [233]

    , keywords =

    The evolution and fate of Very Massive Objects. , keywords =. doi:10.1086/162057 , adsurl =

    doi

  223. [234]

    Non-LTE Models and Theoretical Spectra of Accretion Disks in Active Galactic Nuclei. III. Integrated Spectra for Hydrogen-Helium Disks. , keywords =. doi:10.1086/308708 , archivePrefix =. astro-ph/9911317 , primaryClass =

    doi arXiv

  224. [235]

    , keywords =

    Remarks on the ``Omega -limit''. , keywords =

  225. [236]

    Stellar evolution with rotation. VI. The Eddington and Omega -limits, the rotational mass loss for OB and LBV stars. , keywords =. doi:10.48550/arXiv.astro-ph/0006405 , archivePrefix =. astro-ph/0006405 , primaryClass =

    doi arXiv

  226. [237]

    , year = 1924, month = jun, volume =

    The radiative equilibrium of a rotating system of gaseous masses. , year = 1924, month = jun, volume =. doi:10.1093/mnras/84.9.665 , adsurl =

    1924 doi

  227. [238]

    , year = 1967, month = jan, volume =

    Gravity-Darkening for Stars with Convective Envelopes. , year = 1967, month = jan, volume =

    1967

  228. [239]

    , keywords =

    Numerical simulations of radiatively driven dusty winds. , keywords =. doi:10.1093/mnras/stt1174 , archivePrefix =. 1302.4440 , primaryClass =

    doi arXiv

  229. [240]

    , keywords =

    Radiation Feedback in ULIRGs: Are Photons Movers and Shakers?. , keywords =. doi:10.1088/0004-637X/796/2/107 , archivePrefix =. 1403.1874 , primaryClass =

    doi arXiv

  230. [241]

    , keywords =

    Effects of an Immortal Stellar Population in AGN Disks. , keywords =. doi:10.3847/1538-4357/ac5d40 , archivePrefix =. 2203.06187 , primaryClass =

    doi

  231. [242]

    , keywords =

    Electromagnetic Signatures of Relativistic Explosions in the Disks of Active Galactic Nuclei. , keywords =. doi:10.3847/2041-8213/abd319 , archivePrefix =. 2011.08873 , primaryClass =

    doi

  232. [243]

    , keywords =

    Star-disc interactions near a massive black hole. , keywords =. doi:10.1093/mnras/250.3.505 , adsurl =

    doi

  233. [244]

    , keywords =

    Supernova Explosions in Accretion Disks in Active Galactic Nuclei: Three-dimensional Models. , keywords =. doi:10.3847/1538-4357/abca88 , archivePrefix =. 2011.13877 , primaryClass =

    2011 doi

  234. [245]

    Major AGN flares

    Understanding extreme quasar optical variability with CRTS - I. Major AGN flares. , keywords =. doi:10.1093/mnras/stx1456 , archivePrefix =. 1706.03079 , primaryClass =

    doi arXiv

  235. [246]

    arXiv e-prints , keywords =

    Disks as Inhomogeneous, Anisotropic Gaussian Random Fields. arXiv e-prints , keywords =

  236. [247]

    , keywords =

    Rapid and Bright Stellar-mass Binary Black Hole Mergers in Active Galactic Nuclei. , keywords =. doi:10.3847/1538-4357/835/2/165 , archivePrefix =. 1602.03831 , primaryClass =

    doi arXiv

  237. [248]

    arXiv e-prints , keywords =

    A Family Tree of Optical Transients from Narrow-Line Seyfert 1 Galaxies. arXiv e-prints , keywords =

  238. [249]

    1996 , month =

    , keywords =. 1996 , month =. doi:10.1086/192264 , adsurl =

    1996 doi

  239. [250]

    2010 , month =

    , keywords =. 2010 , month =. doi:10.1088/0067-0049/189/1/240 , adsurl =

    2010 doi

  240. [251]

    2007 , month =

    , archivePrefix =. 2007 , month =. doi:10.1103/PhysRevD.76.025028 , adsurl =. 0707.3500 , keywords =

    2007 doi arXiv

  241. [252]

    Production and growth

    Intermediate mass black holes in AGN discs - I. Production and growth. , keywords =. doi:10.1111/j.1365-2966.2012.21486.x , archivePrefix =. 1206.2309 , primaryClass =

    2012 doi

  242. [253]

    1985 , month =

    , keywords =. 1985 , month =. doi:10.1086/163208 , adsurl =

    1985 doi

  243. [254]

    doi:10.1006/adnd.1994.1007 , adsurl =

    Atomic Data and Nuclear Data Tables , year =. doi:10.1006/adnd.1994.1007 , adsurl =

    1994 doi

  244. [255]

    2000 , month =

    Nuclear Physics A , eprint =. 2000 , month =. doi:10.1016/S0375-9474(00)00131-7 , adsurl =

    2000 doi

  245. [256]

    , keywords =

    Envelope Convection, Surface Magnetism, and Spots in A and Late B-type Stars. , keywords =. doi:10.3847/1538-4357/ab3924 , archivePrefix =. 1904.02161 , primaryClass =

    1904 doi

  246. [257]

    1993 , month =

    , keywords =. 1993 , month =. doi:10.1086/172958 , adsurl =

    1993 doi

  247. [258]

    1996 , month =

    , keywords =. 1996 , month =. doi:10.1086/177381 , adsurl =

    1996 doi

  248. [259]

    , keywords =

    Compton scattering opacities in a partially degenerate electron plasma at high temperatures. , keywords =. doi:10.1086/154847 , adsurl =

    doi

  249. [260]

    , eprint =

    Updated Electron-Conduction Opacities: The Impact on Low-Mass Stellar Models. , eprint =. doi:10.1086/516819 , adsurl =

    doi

  250. [261]

    2005 , month =

    , eprint =. 2005 , month =. doi:10.1086/428642 , adsurl =

    2005 doi

  251. [262]

    The FreeEOS Code for Calculating the Equation of State for Stellar Interiors , url =

  252. [263]

    2000 , month =

    , keywords =. 2000 , month =. doi:10.1086/313304 , adsurl =

    2000 doi

  253. [264]

    1995 , month =

    , keywords =. 1995 , month =. doi:10.1086/192204 , adsurl =

    1995 doi

  254. [265]

    2010 , month =

    Contributions to Plasma Physics , archivePrefix =. 2010 , month =. doi:10.1002/ctpp.201010017 , adsurl =. 1001.0690 , primaryClass =

    2010 doi arXiv

  255. [266]

    , keywords =

    Updated and Expanded OPAL Equation-of-State Tables: Implications for Helioseismology. , keywords =. doi:10.1086/341894 , adsurl =

    doi

  256. [267]

    1983 , month =

    , keywords =. 1983 , month =. doi:10.1086/160960 , adsurl =

    1983 doi

  257. [268]

    1988 , month =

    , keywords =. 1988 , month =

    1988

  258. [269]

    Screening Factors for Nuclear Reactions. I. General Theory. , year = 1973, month = Apr, volume =. doi:10.1086/152061 , adsurl =

    1973 doi

  259. [270]

    Australian Journal of Physics , year = 1954, month = Sep, volume =

    Electrons Screening and Thermonuclear Reactions. Australian Journal of Physics , year = 1954, month = Sep, volume =. doi:10.1071/PH540373 , adsurl =

    1954 doi

  260. [271]

    , keywords =

    Nuclear reaction rate enhancement in dense stellar matter. , keywords =. doi:10.1086/156681 , adsurl =

    doi

  261. [272]

    II - Ionic mixtures

    Enhancement of thermonuclear reaction rate due to strong screening. II - Ionic mixtures. , keywords =. doi:10.1086/157590 , adsurl =

    doi

  262. [273]

    , year = 1958, month = may, volume =

    Completion of the Proton-Proton Reaction Chain and the Possibility of Energetic Neutrino Emission by Hot Stars. , year = 1958, month = may, volume =. doi:10.1086/146487 , adsurl =

    1958 doi

  263. [274]

    doi:10.5281/zenodo.2669541 , month = may, publisher =

    doi

  264. [275]

    J. D. Computing in Science Engineering , title=. 2007 , volume=

    2007

  265. [276]

    Computing in Science Engineering , title=

    S. Computing in Science Engineering , title=. 2011 , volume=

    2011

  266. [277]

    , keywords =

    Orbital Migration of Low-mass Planets in Evolutionary Radiative Models: Avoiding Catastrophic Infall. , keywords =. 2010. doi:10.1088/2041-8205/715/2/L68 , archivePrefix =. 1003.0925 , primaryClass =

    2010 doi arXiv

  267. [278]

    Unsaturated horseshoe drag

    A torque formula for non-isothermal type I planetary migration - I. Unsaturated horseshoe drag. , keywords =. 2010. doi:10.1111/j.1365-2966.2009.15782.x , archivePrefix =. 0909.4552 , primaryClass =

    2010 doi

  268. [279]

    Three-Dimensional Interaction between a Planet and an Isothermal Gaseous Disk. I. Corotation and Lindblad Torques and Planet Migration. , keywords =. 2002. doi:10.1086/324713 , adsurl =

    2002 doi

  269. [280]

    , keywords =

    Local Simulations of Heating Torques on a Luminous Body in an Accretion Disk. , keywords =. doi:10.3847/1538-4357/abb4df , archivePrefix =. 2005.03785 , primaryClass =

    2005 doi

  270. [281]

    , keywords =

    On the Metal Abundance of Low-Activity Galactic Nuclei. , keywords =. doi:10.1086/168109 , adsurl =

    doi

  271. [282]

    , keywords =

    The chemical make-up of the Sun: A 2020 vision. , keywords =. doi:10.1051/0004-6361/202140445 , archivePrefix =. 2105.01661 , primaryClass =

    2020 doi arXiv

  272. [283]

    , keywords =

    Metallicities and Abundance Ratios from Quasar Broad Emission Lines. , keywords =. doi:10.1086/324289 , archivePrefix =. astro-ph/0109006 , primaryClass =

    doi arXiv

  273. [284]

    , keywords =

    De re metallica: the cosmic chemical evolution of galaxies. , keywords =. doi:10.1007/s00159-018-0112-2 , archivePrefix =. 1811.09642 , primaryClass =

    doi arXiv

  274. [285]

    , keywords =

    Nitrogen-Enriched Quasars in the Sloan Digital Sky Survey First Data Release. , keywords =. doi:10.1086/422346 , archivePrefix =. astro-ph/0402205 , primaryClass =

    doi arXiv

  275. [286]

    , keywords =

    A Search for Nitrogen-Enriched Quasars in the Sloan Digital Sky Survey Early Data Release. , keywords =. doi:10.1086/381299 , archivePrefix =. astro-ph/0308486 , primaryClass =

    doi arXiv

  276. [287]

    , keywords =

    A Sample of Quasars with Strong Nitrogen Emission Lines from the Sloan Digital Sky Survey. , keywords =. doi:10.1086/587868 , archivePrefix =. 0802.4234 , primaryClass =

    doi arXiv

  277. [288]

    , keywords =

    The metallicities of the broad emission line regions in the nitrogen-loudest quasars. , keywords =. doi:10.1093/mnras/stu007 , adsurl =

    doi

  278. [289]

    , keywords =

    Chemical evolution of high-redshift radio galaxies. , keywords =. doi:10.1051/0004-6361/200811478 , archivePrefix =. 0905.1581 , primaryClass =

    doi arXiv

  279. [290]

    , keywords =

    A Candidate Tidal Disruption Event in a Quasar at z = 2.359 from Abundance Ratio Variability. , keywords =. doi:10.3847/1538-4357/aabb04 , archivePrefix =. 1803.06362 , primaryClass =

    doi arXiv

  280. [291]

    , keywords =

    Imprint of Accretion Disk-Induced Migration on Gravitational Waves from Extreme Mass Ratio Inspirals. , keywords =. doi:10.1103/PhysRevLett.107.171103 , archivePrefix =. 1103.4609 , primaryClass =

    doi arXiv

  281. [292]

    , keywords =

    Abundance anomalies in tidal disruption events. , keywords =. doi:10.1093/mnras/stw267 , archivePrefix =. 1512.03065 , primaryClass =

    doi arXiv

  282. [293]

    , keywords =

    Stellar Evolution in the Disks of Active Galactic Nuclei Produces Rapidly Rotating Massive Stars. , keywords =. doi:10.3847/1538-4357/abfb67 , archivePrefix =. 2102.13114 , primaryClass =

    doi

  283. [294]

    , keywords =

    Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts. , keywords =. doi:10.1051/0004-6361:20054030 , archivePrefix =. astro-ph/0508242 , primaryClass =

    doi arXiv

  284. [295]

    The ON-blue stragglers

    Evidences for a bifurcation in massive star evolution. The ON-blue stragglers. , keywords =

  285. [296]

    , keywords =

    The Compactness of Presupernova Stellar Cores. , keywords =. doi:10.1088/0004-637X/783/1/10 , archivePrefix =. 1311.6546 , primaryClass =

    doi arXiv

  286. [297]

    , keywords =

    The Progenitor Dependence of the Pre-explosion Neutrino Emission in Core-collapse Supernovae. , keywords =. doi:10.1088/0004-637X/762/2/126 , archivePrefix =. 1207.1100 , primaryClass =

    doi arXiv

  287. [298]

    Monthly Notices of the Royal Astronomical Society: Letters , volume =

    King, Andrew and Nixon, Chris , title = ". Monthly Notices of the Royal Astronomical Society: Letters , volume =. 2015 , month =. doi:10.1093/mnrasl/slv098 , url =

    2015 doi

  288. [299]

    Coevolution of Black Holes and Galaxies , year = 2004, editor =

    QSO Lifetimes. Coevolution of Black Holes and Galaxies , year = 2004, editor =

    2004

  289. [300]

    , year = 1964, month = aug, volume =

    Accretion of Interstellar Matter by Massive Objects. , year = 1964, month = aug, volume =. doi:10.1086/147973 , adsurl =

    1964 doi

Pith tools

Reviewed June 28, 2026 · model on record in the stance chip above.