N-body simulations show gas drag prevents efficient outward scattering of CM-like planetesimals beyond 15 au during Saturn's growth, yielding at most 0.02-0.04 Earth masses of CM material in the outer ring and negligible CI contamination.
Title resolution pending
11 Pith papers cite this work. Polarity classification is still indexing.
11
Pith papers citing it
representative citing papers
A QPO candidate in NGC 1566 supports misaligned accretion flows fueled by captured broad-line region clouds as the cause of rapid changing-look AGN transitions.
MCMC fits to accretion disk SEDs of 23 high-z blazars give black hole masses of 10^8-10^10 solar masses and Eddington ratios 0.04-1, showing that ignoring IGM attenuation overestimates masses with larger bias at higher redshift.
Four infrared-selected young stellar objects are confirmed as FUor eruptions via CO and H2O absorption features, equivalent width diagrams, and disk models showing high extinction and accretion rates comparable to classical FUors.
Multi-planet systems produce size-dependent dust traps, asymmetric structures, and eccentric orbits that can hide gaps in synthetic ALMA images and limit grain growth.
Optical polarimetry shows intrinsic ~0.3% polarization from scattering in the accretion disk wind of Swift J1727.8-1613, with polarization angle offset from the jet indicating black hole spin-orbit misalignment.
Flux eruptions in MADs enhance non-axisymmetry near the black hole via m=1 and m=2 modes driven by vertical magnetic flux bundles formed through reconnection and expelled by buoyancy.
The high-contrast dust asymmetry in HD 34700A is reproduced by a vortex model, with contrast levels excluding eccentric cavity orbit clustering.
Upper limits on the shortest AGN variability timescales are log(t_min,ul/hrs) = 0.85 ± 0.55, interpreted as light-crossing times from a few to thousands of gravitational radii in regions smaller than accretion disks.
Multi-color light curves of TCP J23580961+5502508 reveal early superhumps with a shift from single to two-armed flaring in the accretion disk during the initial rise of the superoutburst.
PS16dtm is the tidal disruption of a 0.3 solar-mass star on a circular counter-rotating orbit inside the accretion disk of an NLS1 galaxy, hidden by a gaseous envelope from the observer's view.
citing papers explorer
-
Shaken, not stirred: inefficient mixing of CM- and CI-like materials
N-body simulations show gas drag prevents efficient outward scattering of CM-like planetesimals beyond 15 au during Saturn's growth, yielding at most 0.02-0.04 Earth masses of CM material in the outer ring and negligible CI contamination.
-
X-ray Quasi-Periodic Oscillations in Active Galactic Nuclei and Their Implications for the Changing Look Phenomenon
A QPO candidate in NGC 1566 supports misaligned accretion flows fueled by captured broad-line region clouds as the cause of rapid changing-look AGN transitions.
-
Black-hole mass estimation through accretion disk spectral fitting for high-redshift blazars
MCMC fits to accretion disk SEDs of 23 high-z blazars give black hole masses of 10^8-10^10 solar masses and Eddington ratios 0.04-1, showing that ignoring IGM attenuation overestimates masses with larger bias at higher redshift.
-
Characterizing and spectrally modeling embedded FUor eruptions in the near-infrared
Four infrared-selected young stellar objects are confirmed as FUor eruptions via CO and H2O absorption features, equivalent width diagrams, and disk models showing high extinction and accretion rates comparable to classical FUors.
-
Dust distribution in circumstellar disks harboring multi-planet systems. II. Super-thermal mass planets
Multi-planet systems produce size-dependent dust traps, asymmetric structures, and eccentric orbits that can hide gaps in synthetic ALMA images and limit grain growth.
-
Optical polarimetry of the accreting black hole X-ray binary Swift J1727.8$-$1613 over the state transition and radio ejections
Optical polarimetry shows intrinsic ~0.3% polarization from scattering in the accretion disk wind of Swift J1727.8-1613, with polarization angle offset from the jet indicating black hole spin-orbit misalignment.
-
The azimuthal structure of magnetically arrested disks during flux eruption events
Flux eruptions in MADs enhance non-axisymmetry near the black hole via m=1 and m=2 modes driven by vertical magnetic flux bundles formed through reconnection and expelled by buoyancy.
-
The Circumbinary Disc of HD 34700A II. Analysis of a strong dust asymmetry
The high-contrast dust asymmetry in HD 34700A is reproduced by a vortex model, with contrast levels excluding eccentric cavity orbit clustering.
-
The shortest detected intra-day variability of active galactic nuclei in TESS survey
Upper limits on the shortest AGN variability timescales are log(t_min,ul/hrs) = 0.85 ± 0.55, interpreted as light-crossing times from a few to thousands of gravitational radii in regions smaller than accretion disks.
-
A growth of early superhump: Multi color observation of the WZ Sge star TCP J23580961+5502508
Multi-color light curves of TCP J23580961+5502508 reveal early superhumps with a shift from single to two-armed flaring in the accretion disk during the initial rise of the superoutburst.
-
Tidal disruption of a low-mass star in an active galactic nucleus as the origin of the PS16dtm outburst
PS16dtm is the tidal disruption of a 0.3 solar-mass star on a circular counter-rotating orbit inside the accretion disk of an NLS1 galaxy, hidden by a gaseous envelope from the observer's view.