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The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae

T0 review · 4 major / 5 minor · reviewed 2026-08-14 · deepseek-v4-flash

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Pith's one-line read Core-collapse supernovae explode inside molecular gas that is roughly two and a half times as turbulent as the average of their host galaxies.

desk verdict The raw signal is real, but the paper's own structure-matched control nullifies the 'unusually turbulent GMC' interpretation. read the letter →

arxiv 2608.08380 v1 pith:MUX6AC3W submitted 2026-08-09 astro-ph.GA astro-ph.HE

M. Solar , M. J. Micha{l}owski , J. Nadolny , J. Sollerman , E. Zapartas , A. Oliva , L. Galbany , J. Hjorth
show 6 more authors
B. Ayala M. Koprowski A. Leśniewska P. Nowaczyk O. Ryzhov B. Šlaus
This is my paper · ORCID
classification astro-ph.GAastro-ph.HE
keywords core-collapsesupernovaemoleculargasturbulenceCO(2-1)velocitydispersiongiantcloudsvirialparameterinterferometricobservationsgalaxies:ISMsupernovae:general
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

Core-collapse supernovae are the deaths of massive stars, and the gas they die inside should carry traces of the clouds their progenitors were born from. This paper measures, for the first time, the turbulence of that molecular gas at the positions of 33 nearby supernovae, using CO(2-1) observations at roughly 100-parsec resolution. It finds that supernova positions sit in molecular gas with median velocity dispersions of about 9.0-9.5 km/s, more than double the 3.81 km/s typical of host-galaxy pixels, and that the excess survives when distances from galaxy centres and host-galaxy structures are taken into account. The authors argue that such turbulent birth environments favour dense-gas formation and binary or multiple stellar systems, which would explain why so many supernova progenitors show signs of binary interaction. If correct, supernova positions become a direct tracer of the most dynamically active giant molecular clouds in nearby galaxies.

What carries the argument

The analysis rests on the CO(2-1) rotational line of carbon monoxide as a tracer of molecular hydrogen, observed at resolutions of roughly 40-230 pc so that individual giant molecular clouds are approached. The turbulence proxy is the velocity dispersion $\sigma_{\rm CO(2-1)}$, the second moment of the CO line profile, measured at each position; the dynamical state is quantified by the virial parameter $\alpha_{\rm vir} = 10\,\sigma^2/(\pi G\,\Sigma_{\rm mol}\,\theta)$, which separates gravitationally bound clouds ($\alpha_{\rm vir} < 2$) from supervirial, dispersing ones ($\alpha_{\rm vir} > 2$). The comparison against a large resolved survey of host-galaxy pixels, together with the scaling relation between velocity dispersion, cloud size, and surface density, lets the paper separate a pure density effect from an excess in turbulence at fixed surface density.

What would settle it

Re-observe the eleven supernova fields currently covered only by 12-metre-array data with full 12m+7m+total-power mosaics and recompute the median CO(2-1) velocity dispersions; if the median drops toward the host-galaxy value of 3.81 km/s once the missing short-spacing flux is restored, the central claim would be falsified for a third of the sample.

Watch

Extended reading notes

Core claim

The central claim is that core-collapse supernovae do not simply occur in dense molecular gas; they occur in molecular gas that is unusually turbulent. From CO(2-1) line observations of 33 supernova positions, 19 hydrogen-rich and 14 stripped-envelope (hydrogen-poor) events, the paper measures median velocity dispersions of $9.0^{+2.0}_{-0.6}$ km/s for hydrogen-rich and $9.5^{+0.3}_{-0.3}$ km/s for stripped-envelope supernovae, compared with $3.81^{+0.01}_{-0.01}$ km/s for the resolved reference pixels of the host galaxies. The corresponding virial parameters are also elevated, $9.5^{+1.3}_{-2.4}$ and $16.1^{+3.3}_{-2.3}$ versus $3.56^{+0.01}_{-0.01}$, indicating that the clouds at explosion sites are not just denser but more strongly dominated by non-thermal, turbulent motion than typical giant molecular clouds. The excess remains after restricting the comparison to similar galactocentric radii and to the same galactic structures, and the authors show that the supernovae themselves could not have produced the measured line widths: even the oldest event would have a shock radius of less than a parsec, far below the 100-pc beam.

Load-bearing premise

The load-bearing assumption is that the velocity dispersions measured at the supernova positions are directly comparable to the reference galaxy pixels: a third of the sample was observed with a single 12-metre array configuration, and if those observations miss about half the CO flux, truncating line wings or selecting only bright compact clumps, the reported turbulence excess could be biased upwards.

Editorial extensions

If this is right

  • Supernova explosion sites trace the high-turbulence tail of the giant-molecular-cloud population, not just the dense tail, so models of massive-star formation must reproduce progenitors emerging preferentially from gas with $\sigma_{\rm CO(2-1)} \sim 9$ km/s.
  • Because the excess persists at fixed gas surface density, turbulence itself, not merely density, correlates with massive-star formation, supporting turbulent-fragmentation and feedback-triggered star-formation scenarios.
  • The elevated virial parameters at supernova positions imply that many parent clouds are supervirial, so the progenitors formed in regions that were dispersing or externally driven rather than quietly collapsing.
  • Hydrogen-rich and stripped-envelope supernovae show similar velocity dispersions, suggesting a common turbulent birth environment, while the slightly higher virial parameters of stripped-envelope events hint at even more extreme clouds (a difference the paper notes is not statistically significant).
  • Because the supernova shocks themselves contribute negligibly to the measured line widths, the turbulence reflects the birth environment and can be used to constrain progenitor formation without subtracting the explosions' own feedback.

Reading between the lines

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

  • One extension the authors do not pursue: if the offset is real, supernova positions could serve as a sparse but unbiased tracer of the most turbulent 100-pc-scale gas across many galaxies, complementing full mapping surveys at a fraction of the observing time.
  • The turbulence-binarity interpretation could be tested by combining these line widths with pre-explosion imaging statistics: it predicts a higher companion-detection rate, or more merger remnants, among progenitors born in the highest-$\sigma_{\rm CO(2-1)}$ clouds.
  • The cleanest confirmation would come from re-observing the 11 twelve-metre-only positions with short-spacing coverage; if the offset shrinks, the result would apply only to the fully mosaicked positions.
  • The same method applied to other transients, such as gamma-ray bursts or superluminous supernovae, would show whether the turbulence excess is specific to core-collapse progenitors or shared by all massive-star explosions.
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Editorial analysis

A structured set of objections, weighed in public.

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

Referee Report

4 major / 5 minor

Summary. The paper analyzes ALMA CO(2-1) observations toward 33 nearby core-collapse supernovae (19 H-rich, 14 SESNe), measuring molecular gas surface density, velocity dispersion, and virial parameter at ~100 pc scales. It compares these values with 150,000 pixels from 15 PHANGS-ALMA galaxies and reports that CCSNe explode in molecular gas with higher velocity dispersion (median 9.0-9.5 km/s vs 3.81 km/s) and higher surface density than the average of the PHANGS pixels. The authors interpret this as evidence that CCSN progenitors form in unusually turbulent GMCs, possibly linked to high gas density or binary nature. The paper includes extensive appendices checking host galaxy properties, radial residuals, and the Σ-σ excess; Appendix B.4 presents a matched-morphology comparison that yields a median excess of +0.002 dex in log σ, a result not reflected in the abstract or conclusions.

Significance. If the central claim were established, this would be a notable new observational constraint on the environments of CCSN progenitors, connecting GMC-scale turbulence to massive star formation channels. The paper is honest in reporting its caveats and includes several useful control analyses. However, the significance of the result is currently limited by the discrepancy between the unmatched comparison (Table 1, Section 3) and the structure-matched control (Appendix B.4), as well as by statistical and sample-comparison issues. The work has value as a catalog and a first attempt, but the headline conclusion as stated is not yet supported by the full evidence presented.

major comments (4)
  1. [Section 3 / Appendix B.4 / Abstract / Section 5] The main claim that CCSN sites are unusually turbulent is contradicted by the paper's own matched-control test. Appendix B.4 reports a median log σ_CO excess of +0.002 dex (16th-84th percentile -0.142 to +0.308) when comparing the 19 PHANGS CCSNe to pixels within the same Querejeta et al. (2021) morphological mask. This null result is mentioned only in one sentence in Section 3 and is absent from the abstract and Section 5 conclusions, where the 'high turbulence' and binary-nature interpretations are featured. Section 4.1 uses the unmatched B.3 excess to argue that 'even at fixed gas surface density, the velocity dispersion at the explosion sites remains significantly higher,' which is not supported by the structure-matched analysis. The authors must either explicitly reconcile this discrepancy, provide a quantitative argument for why the morphological control is not the appropriate reference, or substantially soften the central claim to say that CCSNe are found in dense, high-dispersion regions that are typical of their host galaxy's structure.
  2. [Section 2.1 / Table 1 / Section 3] For 12 of the 33 CCSNe (the ACOS+archival subsample), the reference distribution consists of PHANGS-ALMA pixels from other galaxies rather than the CCSN's own host galaxy. The abstract claims that CCSNe have high velocity dispersion 'compared to the average of their host galaxies,' but this is literally true only for the 21 PHANGS-ALMA CCSNe. Since velocity dispersion depends on galactic environment, mass, and inclination, the cross-galaxy comparison may bias the result. The authors should either restrict the primary statistical comparison to the 21 PHANGS CCSNe, or present a per-host-galaxy analysis that demonstrates the offset persists for the ACOS/archival sample alone.
  3. [Section 3 / Table 2] The KS and AD p-values in Table 2 treat the 150,000 reference pixels as independent draws. Molecular gas is spatially correlated on scales comparable to the beam (~100 pc) and the pixels are clustered within only 15 galaxies; the effective number of independent measurements is far smaller than 150,000. The reported p-values (e.g., 1.57e-5 for SESN σ_CO and 2.50e-7 for SESN α_vir) therefore overstate the significance. The significance of the CCSN-versus-reference differences should be re-evaluated with a scheme that accounts for spatial autocorrelation, for example by bootstrap-resampling spatially independent regions or by using a hierarchical model with galaxy as a random effect.
  4. [Section 4.2] The caveat about missing short-spacing flux is acknowledged, but the statement that missing flux 'would make our conclusion that CCSN sites have higher Σ_mol and σ_CO than the reference regions even stronger' is not justified for σ_CO. For the 11 CCSNe observed with 12m-only data (and 1 with 7m-only), losing ~50% of the total CO flux could truncate broad line wings or select only compact bright clumps, biasing the moment-2 velocity dispersion in either direction. The paper should quantify the sign and magnitude of this bias, for example by comparing σ_CO measured from 12m-only versus 12m+7m+TP maps in the same PHANGS fields, or at minimum rephrase the claim to apply only to Σ_mol and state that the effect on σ_CO is uncertain.
minor comments (5)
  1. [Section 2.2] In the definition of the virial parameter in Eq. (1), the symbol θ is used both for the beam size and later in Eq. (2) for a fixed 100 pc scale; the text should clarify whether θ is the physical beam FWHM or an assumed cloud size, and how the different θ values across the sample affect the comparison.
  2. [Abstract] The phrase 'supports their increased formation in regions of high densities and/or their binary nature' is stronger than the evidence: the observations characterize the current environment, not the birth conditions, and the binary interpretation is one of several plausible scenarios. Softer wording such as 'is consistent with' would be more accurate.
  3. [Appendix B.4] The last paragraph of Section B.4 says the general trends show CCSN molecular gas environments 'share similar properties of the galactic structures,' which is the key null result, but this statement is buried in an appendix; consider moving it to the main text or at least summarizing it in Section 3 with the same emphasis as the unmatched result.
  4. [Figure 1] The caption lists 'typical error bars are denoted as gray, blue, and red' but does not define which symbol corresponds to which color; please clarify the assignment of colors to H-rich SNe, SESNe, and PHANGS-ALMA pixels.
  5. [Table 1] The 1σ confidence intervals for the medians are reported from 10^4 Monte Carlo simulations, but the underlying bootstrap or error-propagation method is not described; a one-sentence explanation in the text or caption would aid reproducibility.

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity: the velocity dispersions, surface densities, and virial parameters at CCSN positions are direct measurements compared against an external PHANGS-ALMA reference sample, with no fitted parameter or load-bearing self-citation determining the reported result.

full rationale

The central quantities are measured rather than derived from the conclusion: sigma_CO(2-1) comes from moment-2 maps and Sigma_mol from integrated CO fluxes, and the virial parameter is computed from the standard formula in Eq. (1) using those measured inputs. The paper does not present alpha_vir as an independent prediction, and the turbulence claim rests on the directly measured sigma offset in Table 1, not on any fitted or predicted quantity. The comparison baseline of 150,000 PHANGS-ALMA pixels is external, and the adopted alpha_CO and R21 values come from independent literature (Bolatto et al. 2013; den Brok et al. 2021). Self-citations such as Solar et al. (2024) supply ACOS survey data and do not carry a uniqueness theorem or an asserted result on which the analysis depends. Appendix B.4's structure-matched excess of +0.002 dex is an internal robustness result that weakens the interpretive claim of unusually turbulent CCSN environments at fixed galactic structure, but that is a correctness or interpretation issue, not circularity: the Table 1 offset is still a measured comparison and is not equivalent by construction to any input parameter. The missing short-spacing flux caveat (Section 4.2, Pety et al. 2013) affects the comparability of some measurements but does not make the result equivalent to its own inputs.

Assumptions & free parameters 0 free parameters · 4 assumptions · 0 invented entities

No free parameters are fitted in this paper; the analysis uses standard conversion factors from the literature, a fixed S/N threshold, and standard statistical tests. The main unexamined inputs are the constancy of the conversion factors, the comparability of heterogeneous ALMA datasets, and the statistical independence of the reference pixels. No new physical entities are introduced.

assumptions (4)
  • domain assumption CO(2-1)-to-CO(1-0) ratio R21=0.65 and CO-to-H2 conversion factor alpha_CO=4.35 Msun pc^-2 (K km/s)^-1 are constant across the sample.
    Adopted in Section 2.2 from den Brok et al. (2021) and Bolatto et al. (2013). Variations toward galaxy centers are acknowledged and could bias Sigma_mol, though the sigma comparison is less sensitive to this.
  • domain assumption The S/N>4 detection threshold selects the same kind of CO-bright gas at CCSN positions and at reference pixels.
    Section 2.1 applies the same strict masking to PHANGS, ACOS, and archival data. If fainter, lower-sigma gas is excluded more at CCSN positions, the offset could be inflated; the authors argue the threshold is standard.
  • domain assumption Single-configuration ACOS/archival observations recover the same CO line profile as PHANGS 12m+7m+TP observations.
    Assumed when comparing sigma values from mixed datasets. Pety et al. (2013), cited in Section 4.2, estimates about 50% of flux can be missing without compact arrays or total power, so this assumption is load-bearing for the 11 12m-only and 1 7m-only CCSNe.
  • domain assumption The 150,000 reference pixels can be treated as independent samples in the KS and AD tests.
    Section 2.2 draws 10,000 random pixels per PHANGS galaxy. Within a galaxy, CO pixels are spatially correlated, so the effective independent sample size is far smaller than 150,000; this likely overstates the statistical significance reported in Table 2.

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Cite this review

Pith. "Pith review of The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae." pith.science (2026). https://pith.science/paper/MUX6AC3W

@misc{pith2026260808380,
  author       = {Pith},
  title        = {Pith review of: The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/MUX6AC3W}},
  note         = {Machine review of arXiv:2608.08380}
}
abstract

Context. Study of cold molecular hydrogen gas (hereafter molecular gas) provides crucial insights into its interplay with star-forming regions. However, the connection between molecular gas turbulence and the sites of massive star ($> 8~\rm{M}_{\odot}$) explosions as core-collapse supernovae (CCSNe) remains unexplored. Aims. We measure for the first time the turbulence of molecular gas in environments of CCSNe, with the aim to constrain the nature of their progenitors. Methods. In order to reach spatial resolutions of giant molecular cloud (GMC) sizes ($\sim 100~\rm{pc}$), we collected ALMA carbon monoxide $J = 2 \rightarrow 1$ spectral line ($\sim 230.54~\rm{GHz}$) observations (as a tracer of molecular gas) at the locations of 33 nearby CCSNe ($< 100~\rm{Mpc}$). Results. We found that CCSNe prefer molecular gas regions with high velocity dispersion compared to the average of their host galaxies. Conclusions. For CCSN progenitors, this observational evidence supports their increased formation in regions of high densities and/or their binary nature.

Figures

Figures reproduced from arXiv: 2608.08380 by the authors.

Figure 1
Figure 1. Molecular gas properties for CCSNe and PHANGS-ALMA galaxy pixels: CO(2–1) velocity dispersion ( [PITH_FULL_IMAGE:figures/full_fig_p009_1.png] view at source ↗
Figure 1
Figure 1. This demonstrates that our CCSNe are not solely located in the central regions or outskirts of the galaxies. Host galaxies with [PITH_FULL_IMAGE:figures/full_fig_p015_1.png] view at source ↗

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Works this paper leans on

225 extracted references · 19 canonical work pages

  1. [1]

    Akademiia Nauk SSSR Doklady , year = 1941, month = jan, volume =

    The Local Structure of Turbulence in Incompressible Viscous Fluid for Very Large Reynolds' Numbers. Akademiia Nauk SSSR Doklady , year = 1941, month = jan, volume =

    1941

  2. [2]

    Massey Jr

    Frank J. Massey Jr. , title =. Journal of the American Statistical Association , volume =. 1951 , publisher =. doi:10.1080/01621459.1951.10500769 , URL =

    arXiv 1951

  3. [3]

    T. W. Anderson and D. A. Darling , title =. The Annals of Mathematical Statistics , number =. 1952 , doi =

    1952

  4. [4]

    , year = 1955, month = jan, volume =

    The Luminosity Function and Stellar Evolution. , year = 1955, month = jan, volume =. doi:10.1086/145971 , adsurl =

    doi:10.1086/145971 1955

  5. [5]

    , year = 1959, month = mar, volume =

    The Rate of Star Formation. , year = 1959, month = mar, volume =. doi:10.1086/146614 , adsurl =

    doi:10.1086/146614 1959

  6. [6]

    Biometrika , year = 1970, month = apr, volume =

    Monte Carlo Sampling Methods using Markov Chains and their Applications. Biometrika , year = 1970, month = apr, volume =. doi:10.1093/biomet/57.1.97 , adsurl =

    doi:10.1093/biomet/57.1.97 1970

  7. [7]

    , keywords =

    A theory of the interstellar medium: three components regulated by supernova explosions in an inhomogeneous substrate. , keywords =. doi:10.1086/155667 , adsurl =

    doi:10.1086/155667

  8. [8]

    , keywords =

    Observations of CO(J = 2-1) emission from molecular clouds. , keywords =. doi:10.1086/157237 , adsurl =

    doi:10.1086/157237

Show all 225 references
  1. [9]

    , keywords =

    The type II SN 1979c in M 100 and the distance to the Virgo cluster. , keywords =. doi:10.1086/158755 , adsurl =

    doi

  2. [10]

    , keywords =

    Turbulence and star formation in molecular clouds. , keywords =. doi:10.1093/mnras/194.4.809 , adsurl =

    doi

  3. [11]

    , keywords =

    CO Observations of Southern High-Latitude Clouds. , keywords =. doi:10.1086/164181 , adsurl =

    doi

  4. [12]

    Galaxy Distances and Deviations from Universal Expansion , year = 1986, editor =

    Physical models of supernovae and the distance scale. Galaxy Distances and Deviations from Universal Expansion , year = 1986, editor =

    1986

  5. [13]

    , keywords =

    The Early Spectral Phase of Type Ib Supernovae: Evidence for Helium. , keywords =. doi:10.1086/165283 , adsurl =

    doi

  6. [14]

    , keywords =

    Supernova 1987A. , keywords =. doi:10.1146/annurev.aa.27.090189.003213 , adsurl =

  7. [15]

    , year = 1989, month = dec, volume =

    The Asiago supernova catalogue. , year = 1989, month = dec, volume =

    1989

  8. [16]

    , keywords =

    Multiplicity among Solar Type Stars in the Solar Neighbourhood - Part Two - Distribution of the Orbital Elements in an Unbiased Sample. , keywords =

  9. [17]

    , keywords =

    Pressure-confined Clumps in Magnetized Molecular Clouds. , keywords =. doi:10.1086/171638 , adsurl =

    doi

  10. [18]

    , keywords =

    Multiplicity among M Dwarfs. , keywords =. doi:10.1086/171708 , adsurl =

    doi

  11. [19]

    , keywords =

    On the Virial Theorem for Turbulent Molecular Clouds. , keywords =. doi:10.1086/171946 , adsurl =

    doi

  12. [20]

    , keywords =

    Presupernova Evolution in Massive Interacting Binaries. , keywords =. doi:10.1086/171341 , adsurl =

    doi

  13. [21]

    Third Reference Catalogue of Bright Galaxies

  14. [22]

    , keywords =

    The Progenitor of SN 1987A. , keywords =. doi:10.1086/133043 , adsurl =

    doi

  15. [23]

    , year = 1993, month = oct, volume =

    The ``Type IIb'' Supernova 1993J in M81: A Close Relative of Type Ib Supernovae. , year = 1993, month = oct, volume =. doi:10.1086/187043 , adsurl =

    1993 doi

  16. [24]

    Bulletin d'Information du Centre de Donnees Stellaires , year = 1993, month = jan, volume =

    Sternberg Astronomical Institute supernova catalogue. Bulletin d'Information du Centre de Donnees Stellaires , year = 1993, month = jan, volume =

    1993

  17. [25]

    , keywords =

    The Evolution of Massive Stars Including Mass Loss: Presupernova Models and Explosion. , keywords =. doi:10.1086/172886 , adsurl =

    doi

  18. [26]

    , keywords =

    Capture and Induced Disk Accretion in Young Star Encounters. , keywords =. doi:10.1086/173890 , adsurl =

    doi

  19. [27]

    Extragalactic database. VI. Inclination corrections for spiral galaxies and disk opaqueness in the B-band. , keywords =

  20. [28]

    , year = 1997, month = jan, volume =

    Optical Spectra of Supernovae. , year = 1997, month = jan, volume =. doi:10.1146/annurev.astro.35.1.309 , adsurl =

    1997 doi

  21. [29]

    , keywords =

    The cosmological evolution of the QSO luminosity density and of the star formation rate. , keywords =. doi:10.1046/j.1365-8711.1998.01264.x , archivePrefix =. astro-ph/9710134 , primaryClass =

    1998

  22. [30]

    , keywords =

    The Global Schmidt Law in Star-forming Galaxies. , keywords =. doi:10.1086/305588 , archivePrefix =. astro-ph/9712213 , primaryClass =

    arXiv

  23. [31]

    , keywords =

    The Astronomer's Telegram: A Web-based Short-Notice Publication System for the Professional Astronomical Community. , keywords =. doi:10.1086/316184 , archivePrefix =. astro-ph/9802256 , primaryClass =

    arXiv

  24. [32]

    , keywords =

    The Asiago Supernova Catalogue - 10 years after. , keywords =. doi:10.1051/aas:1999404 , archivePrefix =. astro-ph/9908046 , primaryClass =

    arXiv

  25. [33]

    , keywords =

    The Energy Dissipation Rate of Supersonic, Magnetohydrodynamic Turbulence in Molecular Clouds. , keywords =. doi:10.1086/307784 , archivePrefix =. astro-ph/9809177 , primaryClass =

    arXiv

  26. [34]

    Monte Carlo methods in statistical physics

  27. [35]

    , keywords =

    Winds from Hot Stars. , keywords =. doi:10.1146/annurev.astro.38.1.613 , adsurl =

    doi

  28. [36]

    , keywords =

    Is It Round? Spectropolarimetry of the Type II-p Supernova 1999EM. , keywords =. doi:10.1086/320959 , archivePrefix =. astro-ph/0009285 , primaryClass =

    arXiv

  29. [37]

    , keywords =

    Mass-loss predictions for O and B stars as a function of metallicity. , keywords =. doi:10.1051/0004-6361:20010127 , archivePrefix =. astro-ph/0101509 , primaryClass =

    arXiv

  30. [38]

    Science , keywords =

    The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems. Science , keywords =. doi:10.1126/science.1067524 , archivePrefix =. astro-ph/0201098 , primaryClass =

    arXiv

  31. [39]

    The Optical and Near-Infrared Properties of Galaxies. I. Luminosity and Stellar Mass Functions. , keywords =. doi:10.1086/378847 , archivePrefix =. astro-ph/0302543 , primaryClass =

    arXiv

  32. [40]

    , keywords =

    Interstellar Turbulence I: Observations and Processes. , keywords =. doi:10.1146/annurev.astro.41.011802.094859 , archivePrefix =. astro-ph/0404451 , primaryClass =

    arXiv

  33. [41]

    , keywords =

    The Infrared Array Camera (IRAC) for the Spitzer Space Telescope. , keywords =. doi:10.1086/422843 , archivePrefix =. astro-ph/0405616 , primaryClass =

    arXiv

  34. [42]

    , keywords =

    A Turbulent Interstellar Medium Origin of the Binary Period Distribution. , keywords =. doi:10.1086/380111 , archivePrefix =. astro-ph/0303280 , primaryClass =

    arXiv

  35. [43]

    Simulating star formation in molecular cloud cores. I. The influence of low levels of turbulence on fragmentation and multiplicity. , keywords =. doi:10.1051/0004-6361:20031594 , archivePrefix =. astro-ph/0309829 , primaryClass =

    arXiv

  36. [44]

    , keywords =

    The Universality of Turbulence in Galactic Molecular Clouds. , keywords =. doi:10.1086/425978 , archivePrefix =. astro-ph/0409420 , primaryClass =

    arXiv

  37. [45]

    Reviews of Modern Physics , keywords =

    Control of star formation by supersonic turbulence. Reviews of Modern Physics , keywords =. doi:10.1103/RevModPhys.76.125 , archivePrefix =. astro-ph/0301093 , primaryClass =

    arXiv

  38. [46]

    , keywords =

    The massive binary companion star to the progenitor of supernova 1993J. , keywords =. doi:10.1038/nature02161 , archivePrefix =. astro-ph/0401090 , primaryClass =

    arXiv

  39. [47]

    Astronomy Letters , year = 2004, month = nov, volume =

    The SAI Catalog of Supernovae and Radial Distributions of Supernovae of Various Types in Galaxies. Astronomy Letters , year = 2004, month = nov, volume =. doi:10.1134/1.1819491 , adsurl =

    2004 doi

  40. [48]

    , keywords =

    Interstellar Turbulence II: Implications and Effects. , keywords =. doi:10.1146/annurev.astro.42.120403.143327 , archivePrefix =. astro-ph/0404452 , primaryClass =

  41. [49]

    , keywords =

    Bias-free Measurement of Giant Molecular Cloud Properties. , keywords =. doi:10.1086/502982 , archivePrefix =. astro-ph/0601706 , primaryClass =

    arXiv

  42. [50]

    Revista Mexicana de Astronomia y Astrofisica Conference Series , year = 2007, series =

    Circumstellar Interaction Around Type Ib/c Supernovae and the GRB Connection. Revista Mexicana de Astronomia y Astrofisica Conference Series , year = 2007, series =

    2007

  43. [51]

    , keywords =

    Physical Properties of Wolf-Rayet Stars. , keywords =. doi:10.1146/annurev.astro.45.051806.110615 , archivePrefix =. astro-ph/0610356 , primaryClass =

    arXiv

  44. [52]

    Protostars and Planets V , year = 2007, editor =

    The Fragmentation of Cores and the Initial Binary Population. Protostars and Planets V , year = 2007, editor =. doi:10.48550/arXiv.astro-ph/0603233 , archivePrefix =. astro-ph/0603233 , primaryClass =

    2007 doi arXiv

  45. [53]

    , keywords =

    Theory of Star Formation. , keywords =. doi:10.1146/annurev.astro.45.051806.110602 , archivePrefix =. 0707.3514 , primaryClass =

    arXiv

  46. [54]

    Astronomical Data Analysis Software and Systems XVI , year = 2007, editor =

    CASA Architecture and Applications. Astronomical Data Analysis Software and Systems XVI , year = 2007, editor =

    2007

  47. [55]

    Science , keywords =

    The Triple-Ring Nebula Around SN 1987A: Fingerprint of a Binary Merger. Science , keywords =. doi:10.1126/science.1136351 , archivePrefix =. astro-ph/0703317 , primaryClass =

    arXiv

  48. [56]

    , keywords =

    Re-Examining Larson's Scaling Relationships in Galactic Molecular Clouds. , keywords =. doi:10.1088/0004-637X/699/2/1092 , archivePrefix =. 0809.1397 , primaryClass =

    arXiv

  49. [57]

    , keywords =

    The Palomar Transient Factory: System Overview, Performance, and First Results. , keywords =. doi:10.1086/648598 , archivePrefix =. 0906.5350 , primaryClass =

    arXiv

  50. [58]

    , keywords =

    Exploring the Optical Transient Sky with the Palomar Transient Factory. , keywords =. doi:10.1086/605911 , archivePrefix =. 0906.5355 , primaryClass =

    arXiv

  51. [59]

    Observational constraints on the progenitors of Type II-P supernovae

    The death of massive stars - I. Observational constraints on the progenitors of Type II-P supernovae. , keywords =. doi:10.1111/j.1365-2966.2009.14506.x , archivePrefix =. 0809.0403 , primaryClass =

    2009

  52. [60]

    , keywords =

    Progenitors of Core-Collapse Supernovae. , keywords =. doi:10.1146/annurev-astro-082708-101737 , archivePrefix =. 0908.0700 , primaryClass =

    arXiv

  53. [61]

    Science , keywords =

    The Formation of Population III Binaries from Cosmological Initial Conditions. Science , keywords =. doi:10.1126/science.1173540 , archivePrefix =. 0907.2919 , primaryClass =

    arXiv

  54. [62]

    , keywords =

    The landscape of binary core-collapse supernova progenitors and the late emergence of Wolf Rayet winds. , keywords =. doi:10.1093/mnras/staf884 , archivePrefix =. 2503.01993 , primaryClass =

    arXiv

  55. [63]

    Physics of the Interstellar and Intergalactic Medium

  56. [64]

    , keywords =

    The First Systematic Study of Type Ibc Supernova Multi-band Light Curves. , keywords =. doi:10.1088/0004-637X/741/2/97 , archivePrefix =. 1011.4959 , primaryClass =

    arXiv

  57. [65]

    , keywords =

    Progenitor Diagnostics for Stripped Core-collapse Supernovae: Measured Metallicities at Explosion Sites. , keywords =. doi:10.1088/2041-8205/731/1/L4 , archivePrefix =. 1007.0661 , primaryClass =

    arXiv

  58. [66]

    , keywords =

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

    arXiv

  59. [67]

    , keywords =

    The link between molecular cloud structure and turbulence. , keywords =. doi:10.1051/0004-6361/200913884 , archivePrefix =. 1001.2453 , primaryClass =

    arXiv

  60. [68]

    , keywords =

    Observed fractions of core-collapse supernova types and initial masses of their single and binary progenitor stars. , keywords =. doi:10.1111/j.1365-2966.2011.17229.x , archivePrefix =. 1006.3899 , primaryClass =

    2011

  61. [69]

    , keywords =

    Massive Molecular Outflows and Negative Feedback in ULIRGs Observed by Herschel-PACS. , keywords =. doi:10.1088/2041-8205/733/1/L16 , archivePrefix =. 1105.1731 , primaryClass =

    arXiv

  62. [70]

    , keywords =

    The Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations. , keywords =. doi:10.1088/0004-637X/761/2/156 , archivePrefix =. 1209.2856 , primaryClass =

    arXiv

  63. [71]

    , keywords =

    Presupernova Evolution of Massive Single and Binary Stars. , keywords =. doi:10.1146/annurev-astro-081811-125534 , archivePrefix =. 1206.5443 , primaryClass =

    arXiv

  64. [72]

    , keywords =

    A unified supernova catalogue. , keywords =. doi:10.1051/0004-6361/201117666 , archivePrefix =. 1112.3592 , primaryClass =

    arXiv

  65. [73]

    Science , keywords =

    Binary Interaction Dominates the Evolution of Massive Stars. Science , keywords =. doi:10.1126/science.1223344 , archivePrefix =. 1207.6397 , primaryClass =

    arXiv

  66. [74]

    , keywords =

    Toward a Complete Accounting of Energy and Momentum from Stellar Feedback in Galaxy Formation Simulations. , keywords =. doi:10.1088/0004-637X/770/1/25 , archivePrefix =. 1210.4957 , primaryClass =

    arXiv

  67. [75]

    , keywords =

    The CO-to-H _ 2 Conversion Factor. , keywords =. doi:10.1146/annurev-astro-082812-140944 , archivePrefix =. 1301.3498 , primaryClass =

    arXiv

  68. [76]

    , keywords =

    Stellar Multiplicity. , keywords =. doi:10.1146/annurev-astro-081710-102602 , archivePrefix =. 1303.3028 , primaryClass =

    arXiv

  69. [77]

    Observational constraints on the progenitors of Type Ibc supernovae

    The death of massive stars - II. Observational constraints on the progenitors of Type Ibc supernovae. , keywords =. doi:10.1093/mnras/stt1612 , archivePrefix =. 1301.1975 , primaryClass =

    1975 arXiv

  70. [78]

    , keywords =

    CO J = 1-0 and J = 2-1 Line Observations of the Molecular-cloud-blocked Supernova Remnant 3C434.1. , keywords =. doi:10.1088/0004-637X/770/2/105 , archivePrefix =. 1305.0771 , primaryClass =

    arXiv

  71. [79]

    , keywords =

    Molecular Gas and Star Formation in nearby Disk Galaxies. , keywords =. doi:10.1088/0004-6256/146/2/19 , archivePrefix =. 1301.2328 , primaryClass =

    arXiv

  72. [80]

    Planets, Stars and Stellar Systems

    Evolution of Active Galactic Nuclei. Planets, Stars and Stellar Systems. Volume 6: Extragalactic Astronomy and Cosmology , year = 2013, editor =. doi:10.1007/978-94-007-5609-0_11 , adsurl =

    2013 doi

  73. [81]

    , keywords =

    The Plateau de Bure + 30 m Arcsecond Whirlpool Survey Reveals a Thick Disk of Diffuse Molecular Gas in the M51 Galaxy. , keywords =. doi:10.1088/0004-637X/779/1/43 , archivePrefix =. 1304.1396 , primaryClass =

    arXiv

  74. [82]

    , keywords =

    The CO-to-H _ 2 Conversion Factor and Dust-to-gas Ratio on Kiloparsec Scales in Nearby Galaxies. , keywords =. doi:10.1088/0004-637X/777/1/5 , archivePrefix =. 1212.1208 , primaryClass =

    arXiv

  75. [83]

    Supernova Environmental Impacts , year = 2014, editor =

    Molecular Environments of Supernova Remnants. Supernova Environmental Impacts , year = 2014, editor =. doi:10.1017/S1743921313009423 , archivePrefix =. 1304.5367 , primaryClass =

    2014 arXiv

  76. [84]

    , keywords =

    Massive molecular outflows and evidence for AGN feedback from CO observations. , keywords =. doi:10.1051/0004-6361/201322464 , archivePrefix =. 1311.2595 , primaryClass =

    arXiv

  77. [85]

    , keywords =

    Uncovering the Putative B-star Binary Companion of the SN 1993J Progenitor. , keywords =. doi:10.1088/0004-637X/790/1/17 , archivePrefix =. 1405.4863 , primaryClass =

    arXiv

  78. [86]

    , keywords =

    Two -ray bursts from dusty regions with little molecular gas. , keywords =. doi:10.1038/nature13325 , archivePrefix =. 1406.3071 , primaryClass =

    arXiv

  79. [87]

    HyperLEDA. III. The catalogue of extragalactic distances. , keywords =. doi:10.1051/0004-6361/201423496 , archivePrefix =. 1408.3476 , primaryClass =

    arXiv

  80. [88]

    , keywords =

    Statistical Studies of Supernova Environments. , keywords =. doi:10.1017/pasa.2015.19 , archivePrefix =. 1504.04043 , primaryClass =

    2015 arXiv

  81. [89]

    , keywords =

    A Classical Morphological Analysis of Galaxies in the Spitzer Survey of Stellar Structure in Galaxies (S4G). , keywords =. doi:10.1088/0067-0049/217/2/32 , archivePrefix =. 1501.00454 , primaryClass =

    arXiv

  82. [90]

    , keywords =

    Inefficient star formation through turbulence, magnetic fields and feedback. , keywords =. doi:10.1093/mnras/stv941 , archivePrefix =. 1504.03690 , primaryClass =

    arXiv

  83. [91]

    , keywords =

    A census of dense cores in the Aquila cloud complex: SPIRE/PACS observations from the Herschel Gould Belt survey. , keywords =. doi:10.1051/0004-6361/201525861 , archivePrefix =. 1507.05926 , primaryClass =

    arXiv

  84. [92]

    , keywords =

    The stellar wind velocity field of HD 77581. , keywords =. doi:10.1051/0004-6361/201526893 , archivePrefix =. 1507.01016 , primaryClass =

    arXiv

  85. [93]

    , keywords =

    Did the progenitor of SN 2011dh have a binary companion? ^ ★. , keywords =. doi:10.1093/mnras/stv2098 , archivePrefix =. 1509.06018 , primaryClass =

    arXiv

  86. [94]

    , keywords =

    Neutrino-driven Supernova of a Low-mass Iron-core Progenitor Boosted by Three-dimensional Turbulent Convection. , keywords =. doi:10.1088/2041-8205/801/2/L24 , archivePrefix =. 1501.01961 , primaryClass =

    arXiv

  87. [95]

    , keywords =

    Neutrino-driven Explosion of a 20 Solar-mass Star in Three Dimensions Enabled by Strange-quark Contributions to Neutrino-Nucleon Scattering. , keywords =. doi:10.1088/2041-8205/808/2/L42 , archivePrefix =. 1504.07631 , primaryClass =

    arXiv

  88. [96]

    , year = 2015, month = feb, volume =

    The formation of a quadruple star system with wide separation. , year = 2015, month = feb, volume =. doi:10.1038/nature14166 , adsurl =

    2015 doi

  89. [97]

    , keywords =

    Observational Constraints on the Progenitors of Core-Collapse Supernovae: The Case for Missing High-Mass Stars. , keywords =. doi:10.1017/pasa.2015.17 , archivePrefix =. 1504.02635 , primaryClass =

    2015 arXiv

  90. [98]

    , keywords =

    A Detection of Molecular Gas Emission in the Host Galaxy of GRB 080517. , keywords =. doi:10.1088/2041-8205/798/1/L7 , archivePrefix =. 1411.7389 , primaryClass =

    arXiv

  91. [99]

    , keywords =

    GRB 980425 host: [C II], [O I], and CO lines reveal recent enhancement of star formation due to atomic gas inflow. , keywords =. doi:10.1051/0004-6361/201629441 , archivePrefix =. 1609.01742 , primaryClass =

    arXiv

  92. [100]

    , keywords =

    A Portrait of Cold Gas in Galaxies at 60 pc Resolution and a Simple Method to Test Hypotheses That Link Small-scale ISM Structure to Galaxy-scale Processes. , keywords =. doi:10.3847/0004-637X/831/1/16 , archivePrefix =. 1606.07077 , primaryClass =

    arXiv

  93. [101]

    Supernova Driving. I. The Origin of Molecular Cloud Turbulence. , keywords =. doi:10.3847/0004-637X/822/1/11 , archivePrefix =. 1509.04663 , primaryClass =

    arXiv

  94. [102]

    Julia: A fresh approach to numerical computing , author=. SIAM. 2017 , publisher=. doi:10.1137/141000671 , url=

    2017 doi

  95. [103]

    , keywords =

    The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMA. , keywords =. doi:10.3847/1538-4357/aa86aa , archivePrefix =. 1704.02504 , primaryClass =

    arXiv

  96. [104]

    , keywords =

    Considering the Single and Binary Origins of the Type IIP SN 2017eaw. , keywords =. doi:10.3847/1538-3881/acffc7 , archivePrefix =. 2310.01498 , primaryClass =

    arXiv

  97. [105]

    , keywords =

    Molecular gas in supernova local environments unveiled by EDGE. , keywords =. doi:10.1093/mnras/stx367 , archivePrefix =. 1702.02945 , primaryClass =

    arXiv

  98. [106]

    , keywords =

    An Open Catalog for Supernova Data. , keywords =. doi:10.3847/1538-4357/835/1/64 , archivePrefix =. 1605.01054 , primaryClass =

    arXiv

  99. [107]

    , keywords =

    The quest for blue supergiants: binary merger models for the evolution of the progenitor of SN 1987A. , keywords =. doi:10.1093/mnras/stx818 , archivePrefix =. 1703.04918 , primaryClass =

    arXiv

  100. [108]

    , keywords =

    Mind Your Ps and Qs: The Interrelation between Period (P) and Mass-ratio (Q) Distributions of Binary Stars. , keywords =. doi:10.3847/1538-4365/aa6fb6 , archivePrefix =. 1606.05347 , primaryClass =

    arXiv

  101. [109]

    , keywords =

    Delay-time distribution of core-collapse supernovae with late events resulting from binary interaction. , keywords =. doi:10.1051/0004-6361/201629685 , archivePrefix =. 1701.07032 , primaryClass =

    arXiv

  102. [110]

    , keywords =

    A molecular gas-rich GRB host galaxy at the peak of cosmic star formation. , keywords =. doi:10.1093/mnras/sty194 , archivePrefix =. 1709.00424 , primaryClass =

    arXiv

  103. [111]

    , keywords =

    A Search for Molecular Gas in the Host Galaxy of FRB 121102. , keywords =. doi:10.3847/1538-3881/aabc5a , archivePrefix =. 1804.01584 , primaryClass =

    arXiv

  104. [112]

    , keywords =

    Connecting young star clusters to CO molecular gas in NGC 7793 with ALMA-LEGUS. , keywords =. doi:10.1093/mnras/sty2154 , archivePrefix =. 1808.02496 , primaryClass =

    arXiv

  105. [113]

    , keywords =

    Relativistic supernova 2009bb exploded close to an atomic gas cloud. , keywords =. doi:10.1051/0004-6361/201732356 , archivePrefix =. 1808.00977 , primaryClass =

    arXiv

  106. [114]

    , keywords =

    Molecular gas masses of gamma-ray burst host galaxies. , keywords =. doi:10.1051/0004-6361/201833250 , archivePrefix =. 1804.06492 , primaryClass =

    arXiv

  107. [115]

    , keywords =

    Is Molecular Cloud Turbulence Driven by External Supernova Explosions?. , keywords =. doi:10.3847/1538-4357/aaacff , archivePrefix =. 1802.00973 , primaryClass =

    arXiv

  108. [116]

    , keywords =

    A Superluminous Supernova in High Surface Density Molecular Gas within the Bar of a Metal-rich Galaxy. , keywords =. doi:10.3847/1538-4357/ab2897 , archivePrefix =. 1906.00972 , primaryClass =

    1906 arXiv

  109. [117]

    , keywords =

    Photometric and spectroscopic diversity of Type II supernovae. , keywords =. doi:10.1051/0004-6361/201935100 , archivePrefix =. 1908.02973 , primaryClass =

    1908 arXiv

  110. [118]

    , keywords =

    Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback. , keywords =. doi:10.1038/s41586-019-1194-3 , archivePrefix =. 1905.08801 , primaryClass =

    1905 arXiv

  111. [119]

    , keywords =

    Star Clusters Across Cosmic Time. , keywords =. doi:10.1146/annurev-astro-091918-104430 , archivePrefix =. 1812.01615 , primaryClass =

    arXiv

  112. [120]

    A z = 0 Multiwavelength Galaxy Synthesis. I. A WISE and GALEX Atlas of Local Galaxies. , keywords =. doi:10.3847/1538-4365/ab3925 , archivePrefix =. 1910.13470 , primaryClass =

    1910 arXiv

  113. [121]

    , keywords =

    ALMA Observations of Molecular Gas in the Host Galaxy of AT2018cow. , keywords =. doi:10.3847/2041-8213/ab2915 , archivePrefix =. 1906.05446 , primaryClass =

    1906 arXiv

  114. [122]

    , keywords =

    A comparison of explosion energies for simulated and observed core-collapse supernovae. , keywords =. doi:10.1093/mnras/stz2123 , archivePrefix =. 1904.09444 , primaryClass =

    1904 arXiv

  115. [123]

    A study of the kinematical imprints of the physical processes governing the evolution and explosion of their binary progenitors

    Massive runaway and walkaway stars. A study of the kinematical imprints of the physical processes governing the evolution and explosion of their binary progenitors. , keywords =. doi:10.1051/0004-6361/201833297 , archivePrefix =. 1804.09164 , primaryClass =

    arXiv

  116. [124]

    , keywords =

    Core-collapse supernovae ages and metallicities from emission-line diagnostics of nearby stellar populations. , keywords =. doi:10.1093/mnras/sty2557 , archivePrefix =. 1805.01213 , primaryClass =

    arXiv

  117. [125]

    , keywords =

    The diverse lives of progenitors of hydrogen-rich core-collapse supernovae: the role of binary interaction. , keywords =. doi:10.1051/0004-6361/201935854 , archivePrefix =. 1907.06687 , primaryClass =

    1907 arXiv

  118. [126]

    , keywords =

    Collisional N-body Dynamics Coupled to Self-gravitating Magnetohydrodynamics Reveals Dynamical Binary Formation. , keywords =. doi:10.3847/1538-4357/ab4db1 , archivePrefix =. 1901.01132 , primaryClass =

    1901 arXiv

  119. [127]

    , keywords =

    Evidence for supernova feedback sustaining gas turbulence in nearby star-forming galaxies. , keywords =. doi:10.1051/0004-6361/202038223 , archivePrefix =. 2006.10764 , primaryClass =

    2006 arXiv

  120. [128]

    , keywords =

    The lifecycle of molecular clouds in nearby star-forming disc galaxies. , keywords =. doi:10.1093/mnras/stz3525 , archivePrefix =. 1911.03479 , primaryClass =

    1911 arXiv

  121. [129]

    A detailed host analysis using ALMA, the HST, and the VLT

    GRB 190114C in the nuclear region of an interacting galaxy. A detailed host analysis using ALMA, the HST, and the VLT. , keywords =. doi:10.1051/0004-6361/201936668 , archivePrefix =. 1911.07876 , primaryClass =

    1911 arXiv

  122. [130]

    , keywords =

    Supernovae Ib and Ic from the explosion of helium stars. , keywords =. doi:10.1051/0004-6361/202038763 , archivePrefix =. 2008.07601 , primaryClass =

    2008 arXiv

  123. [131]

    , keywords =

    Spatially resolved molecular gas properties of host galaxy of Type I superluminous supernova SN 2017egm. , keywords =. doi:10.1093/pasj/psaa052 , archivePrefix =. 2005.06656 , primaryClass =

    2005 arXiv

  124. [132]

    ALMA CO Observations of the Host Galaxies of Long-duration Gamma-Ray Bursts. I. Molecular Gas Scaling Relations. , keywords =. doi:10.3847/1538-4357/ab7992 , archivePrefix =. 2002.09121 , primaryClass =

    2002 arXiv

  125. [133]

    , keywords =

    Systematic Variations of CO J = 2-1/1-0 Ratio and Their Implications in The Nearby Barred Spiral Galaxy M83. , keywords =. doi:10.3847/2041-8213/ab70b7 , archivePrefix =. 2001.11043 , primaryClass =

    2001 arXiv

  126. [134]

    , keywords =

    The Origin of Elements from Carbon to Uranium. , keywords =. doi:10.3847/1538-4357/abae65 , archivePrefix =. 2008.04660 , primaryClass =

    2008 arXiv

  127. [135]

    , keywords =

    PHANGS CO Kinematics: Disk Orientations and Rotation Curves at 150 pc Resolution. , keywords =. doi:10.3847/1538-4357/ab9953 , archivePrefix =. 2005.11709 , primaryClass =

    2005 arXiv

  128. [136]

    , keywords =

    The Effect of Supernovae on the Turbulence and Dispersal of Molecular Clouds. , keywords =. doi:10.3847/1538-4357/abbd8f , archivePrefix =. 2007.09518 , primaryClass =

    2007 arXiv

  129. [137]

    , keywords =

    Connection of supernovae 2002ap, 2003gd, 2013ej, and 2019krl in M 74 with atomic gas accretion and spiral structure. , keywords =. doi:10.1051/0004-6361/202037692 , archivePrefix =. 2004.11391 , primaryClass =

    2004 arXiv

  130. [138]

    , keywords =

    An ALMA CO(2-1) Survey of Nearby Palomar-Green Quasars. , keywords =. doi:10.3847/1538-4365/ab5db2 , archivePrefix =. 1912.00085 , primaryClass =

    1912 arXiv

  131. [139]

    , keywords =

    AGN Feedback and Star Formation of Quasar Host Galaxies: Insights from the Molecular Gas. , keywords =. doi:10.3847/1538-4357/aba8a1 , archivePrefix =. 2007.11286 , primaryClass =

    2007 arXiv

  132. [140]

    , keywords =

    Molecular Gas Properties on Cloud Scales across the Local Star-forming Galaxy Population. , keywords =. doi:10.3847/2041-8213/abb3be , archivePrefix =. 2009.01842 , primaryClass =

    2009 arXiv

  133. [141]

    , keywords =

    Multiscale dynamics in star-forming regions: the interplay between gravity and turbulence. , keywords =. doi:10.1093/mnras/stz3344 , archivePrefix =. 1912.00031 , primaryClass =

    1912 arXiv

  134. [142]

    , keywords =

    Type Ic supernovae from the (intermediate) Palomar Transient Factory. , keywords =. doi:10.1051/0004-6361/202038890 , adsurl =

    doi

  135. [143]

    , keywords =

    The Radio Luminosity-risetime Function of Core-collapse Supernovae. , keywords =. doi:10.3847/1538-4357/abccd9 , archivePrefix =. 2011.11737 , primaryClass =

    2011 arXiv

  136. [144]

    , keywords =

    ALMA Host Galaxy Observation of the Off-axis Gamma-Ray Burst XRF 020903. , keywords =. doi:10.3847/1538-4357/ac00b4 , archivePrefix =. 2105.05508 , primaryClass =

    arXiv

  137. [145]

    CARTA: Cube Analysis and Rendering Tool for Astronomy

  138. [146]

    , keywords =

    New constraints on the ^ 12 CO(2-1)/(1-0) line ratio across nearby disc galaxies. , keywords =. doi:10.1093/mnras/stab859 , archivePrefix =. 2103.10442 , primaryClass =

    arXiv

  139. [147]

    , keywords =

    Different to the core: The pre-supernova structures of massive single and binary-stripped stars. , keywords =. doi:10.1051/0004-6361/202140506 , archivePrefix =. 2102.05036 , primaryClass =

    arXiv

  140. [148]

    , keywords =

    PHANGS-ALMA Data Processing and Pipeline. , keywords =. doi:10.3847/1538-4365/abec80 , archivePrefix =. 2104.07665 , primaryClass =

    arXiv

  141. [149]

    , keywords =

    PHANGS-ALMA: Arcsecond CO(2-1) Imaging of Nearby Star-forming Galaxies. , keywords =. doi:10.3847/1538-4365/ac17f3 , archivePrefix =. 2104.07739 , primaryClass =

    arXiv

  142. [150]

    , keywords =

    Stellar structures, molecular gas, and star formation across the PHANGS sample of nearby galaxies. , keywords =. doi:10.1051/0004-6361/202140695 , archivePrefix =. 2109.04491 , primaryClass =

  143. [151]

    The Palomar Transient Factory Core-collapse Supernova Host-galaxy Sample. I. Host-galaxy Distribution Functions and Environment Dependence of Core-collapse Supernovae. , keywords =. doi:10.3847/1538-4365/abff5e , archivePrefix =. 2008.05988 , primaryClass =

    arXiv

  144. [152]

    CO Multi-line Imaging of Nearby Galaxies (COMING). IX. ^ 12 CO(J = 2-1)/ ^ 12 CO(J = 1-0) line ratio on kiloparsec scales. , keywords =. doi:10.1093/pasj/psaa119 , archivePrefix =. 2012.08523 , primaryClass =

    2012 arXiv

  145. [153]

    , keywords =

    Revisiting the explodability of single massive star progenitors of stripped-envelope supernovae. , keywords =. doi:10.1051/0004-6361/202141506 , archivePrefix =. 2106.05228 , primaryClass =

    arXiv

  146. [154]

    , keywords =

    Effect of binary evolution on the inferred initial and final core masses of hydrogen-rich, Type II supernova progenitors. , keywords =. doi:10.1051/0004-6361/202037744 , archivePrefix =. 2002.07230 , primaryClass =

    2002 arXiv

  147. [155]

    Research in Astronomy and Astrophysics , keywords =

    Spatially resolved properties of supernova host galaxies in SDSS-IV MaNGA. Research in Astronomy and Astrophysics , keywords =. doi:10.1088/1674-4527/21/12/306 , archivePrefix =. 2109.12366 , primaryClass =

    arXiv

  148. [156]

    , keywords =

    CASA, the Common Astronomy Software Applications for Radio Astronomy. , keywords =. doi:10.1088/1538-3873/ac9642 , archivePrefix =. 2210.02276 , primaryClass =

    arXiv

  149. [157]

    , keywords =

    The Candidate Progenitor Companion Star of the Type Ib/c SN 2013ge. , keywords =. doi:10.3847/2041-8213/ac5890 , archivePrefix =. 2203.01357 , primaryClass =

    arXiv

  150. [158]

    , keywords =

    Environmental dependence of the molecular cloud lifecycle in 54 main-sequence galaxies. , keywords =. doi:10.1093/mnras/stac2339 , archivePrefix =. 2206.09857 , primaryClass =

    arXiv

  151. [159]

    , keywords =

    Diverse Properties of Molecular Gas in the Host Galaxies of Fast Radio Bursts. , keywords =. doi:10.3847/2041-8213/ac9f39 , archivePrefix =. 2211.02279 , primaryClass =

    arXiv

  152. [160]

    , keywords =

    PHANGS: constraining star formation time-scales using the spatial correlations of star clusters and giant molecular clouds. , keywords =. doi:10.1093/mnras/stac2559 , archivePrefix =. 2209.02872 , primaryClass =

    arXiv

  153. [161]

    , keywords =

    PHANGS-JWST First Results: Multiwavelength View of Feedback-driven Bubbles (the Phantom Voids) across NGC 628. , keywords =. doi:10.3847/2041-8213/aca7b9 , archivePrefix =. 2212.00812 , primaryClass =

    arXiv

  154. [162]

    arXiv e-prints , keywords =

    Constraining the Molecular Gas Content of Fast Radio Burst (FRB) Host Galaxies. arXiv e-prints , keywords =. doi:10.48550/arXiv.2304.10377 , archivePrefix =. 2304.10377 , primaryClass =

    doi arXiv

  155. [163]

    , keywords =

    The molecular gas kinematics in the host galaxy of non-repeating FRB 180924B. , keywords =. doi:10.1093/mnras/stac3655 , archivePrefix =. 2212.04027 , primaryClass =

    arXiv

  156. [164]

    , keywords =

    SN 2023ixf in Messier 101: A Variable Red Supergiant as the Progenitor Candidate to a Type II Supernova. , keywords =. doi:10.3847/2041-8213/ace4ca , archivePrefix =. 2306.04722 , primaryClass =

    arXiv

  157. [165]

    , keywords =

    The contribution of binary star formation via core fragmentation on protostellar multiplicity. , keywords =. doi:10.1051/0004-6361/202244882 , archivePrefix =. 2209.01909 , primaryClass =

    arXiv

  158. [166]

    Protostars and Planets VII , year = 2023, editor =

    The Origin and Evolution of Multiple Star Systems. Protostars and Planets VII , year = 2023, editor =. doi:10.48550/arXiv.2203.10066 , archivePrefix =. 2203.10066 , primaryClass =

    2023 doi arXiv

  159. [167]

    , keywords =

    Comparing the Locations of Supernovae to CO (2-1) Emission in Their Host Galaxies. , keywords =. doi:10.3847/1538-4357/acab00 , archivePrefix =. 2212.09766 , primaryClass =

    arXiv

  160. [168]

    , keywords =

    SN 2022jli: A Type Ic Supernova with Periodic Modulation of Its Light Curve and an Unusually Long Rise. , keywords =. doi:10.3847/2041-8213/acfc25 , archivePrefix =. 2309.12750 , primaryClass =

    arXiv

  161. [169]

    , keywords =

    Main Sequence to Starburst Transitioning Galaxies: Gamma-Ray Burst Hosts at z 2. , keywords =. doi:10.3847/1538-4357/acd74f , archivePrefix =. 2305.13436 , primaryClass =

    arXiv

  162. [170]

    , keywords =

    The ALMOND survey: molecular cloud properties and gas density tracers across 25 nearby spiral galaxies with ALMA. , keywords =. doi:10.1093/mnras/stad424 , archivePrefix =. 2302.03042 , primaryClass =

    arXiv

  163. [171]

    , keywords =

    Clusters, clouds, and correlations: relating young clusters to giant molecular clouds in M33 and M31. , keywords =. doi:10.1093/mnras/stad1430 , archivePrefix =. 2305.03618 , primaryClass =

    arXiv

  164. [172]

    arXiv e-prints , keywords =

    Where do stars explode in the ISM? -- The distribution of dense gas around massive stars and supernova remnants in M33. arXiv e-prints , keywords =. doi:10.48550/arXiv.2310.17694 , archivePrefix =. 2310.17694 , primaryClass =

    doi

  165. [173]

    ALMA Observations of Supernova Remnant N49 in the Large Magellanic Cloud. II. Non-LTE Analysis of Shock-heated Molecular Clouds. , keywords =. doi:10.3847/1538-4357/acffbe , archivePrefix =. 2311.02180 , primaryClass =

    arXiv

  166. [174]

    , keywords =

    An environmental analysis of the fast transient AT2018cow and implications for its progenitor and late-time brightness. , keywords =. doi:10.1093/mnras/stac3773 , archivePrefix =. 2210.01144 , primaryClass =

    arXiv

  167. [175]

    , keywords =

    PHANGS-JWST First Results: A Statistical View on Bubble Evolution in NGC 628. , keywords =. doi:10.3847/2041-8213/aca6e4 , archivePrefix =. 2212.00811 , primaryClass =

    arXiv

  168. [176]

    , keywords =

    Quantifying the energetics of molecular superbubbles in PHANGS galaxies. , keywords =. doi:10.1051/0004-6361/202346075 , archivePrefix =. 2302.03699 , primaryClass =

    arXiv

  169. [177]

    , keywords =

    Wide-binary Stars Formed in the Turbulent Interstellar Medium. , keywords =. doi:10.3847/2041-8213/acd6f7 , archivePrefix =. 2303.16224 , primaryClass =

    arXiv

  170. [178]

    arXiv e-prints , keywords =

    POSYDON Version 2: Population Synthesis with Detailed Binary-Evolution Simulations across a Cosmological Range of Metallicities. arXiv e-prints , keywords =. doi:10.48550/arXiv.2411.02376 , archivePrefix =. 2411.02376 , primaryClass =

    doi arXiv

  171. [179]

    , keywords =

    JWST Reveals a Luminous Infrared Source at the Position of the Failed Supernova Candidate N6946-BH1. , keywords =. doi:10.3847/1538-4357/ad21fa , archivePrefix =. 2309.16121 , primaryClass =

    arXiv

  172. [180]

    , keywords =

    The progenitor of SN 2023ixf from hydrodynamical modeling. , keywords =. doi:10.1051/0004-6361/202348183 , archivePrefix =. 2310.14407 , primaryClass =

    arXiv

  173. [181]

    arXiv e-prints , keywords =

    HI and CO spectroscopy of the unusual host of GRB 171205A: A grand design spiral galaxy with a distorted HI field. arXiv e-prints , keywords =. doi:10.48550/arXiv.2406.16726 , archivePrefix =. 2406.16726 , primaryClass =

    doi arXiv

  174. [182]

    , keywords =

    A 12.4-day periodicity in a close binary system after a supernova. , keywords =. doi:10.1038/s41586-023-06787-x , archivePrefix =. 2310.07784 , primaryClass =

    arXiv

  175. [183]

    arXiv e-prints , keywords =

    Unveiling the nature of SN 2022jli: the first double-peaked stripped-envelope supernova showing periodic undulations and dust emission at late times. arXiv e-prints , keywords =. doi:10.48550/arXiv.2410.21381 , archivePrefix =. 2410.21381 , primaryClass =

    doi

  176. [184]

    , keywords =

    Probing Presupernova Mass Loss in Double-peaked Type Ibc Supernovae from the Zwicky Transient Facility. , keywords =. doi:10.3847/1538-4357/ad595f , archivePrefix =. 2306.04698 , primaryClass =

    arXiv

  177. [185]

    , keywords =

    The Evolution of Massive Binary Stars. , keywords =. doi:10.1146/annurev-astro-052722-105936 , archivePrefix =. 2311.01865 , primaryClass =

    arXiv

  178. [186]

    , keywords =

    H Emission and H II Regions at the Locations of Recent Supernovae in Nearby Galaxies. , keywords =. doi:10.3847/1538-3881/ad3fb7 , archivePrefix =. 2404.10762 , primaryClass =

    arXiv

  179. [187]

    , keywords =

    The progenitor star of SN 2023ixf: a massive red supergiant with enhanced, episodic pre-supernova mass loss. , keywords =. doi:10.1093/mnras/stae2012 , archivePrefix =. 2309.10022 , primaryClass =

    arXiv

  180. [188]

    , keywords =

    Pre-supernova evolution and final fate of stellar mergers and accretors of binary mass transfer. , keywords =. doi:10.1051/0004-6361/202347854 , archivePrefix =. 2403.03984 , primaryClass =

    arXiv

  181. [189]

    , keywords =

    Molecular Gas and the Star-Formation Process on Cloud Scales in Nearby Galaxies. , keywords =. doi:10.1146/annurev-astro-071221-052651 , archivePrefix =. 2403.19843 , primaryClass =

    arXiv

  182. [190]

    Nature Communications , keywords =

    Binary progenitor systems for Type Ic supernovae. Nature Communications , keywords =. doi:10.1038/s41467-024-51863-z , archivePrefix =. 2409.01906 , primaryClass =

    arXiv

  183. [191]

    , keywords =

    The turbulent support and global hierarchical collapse models for molecular clouds compared: differences, convergence, and myths. , keywords =. doi:10.1093/mnras/staf2059 , archivePrefix =. 2408.10406 , primaryClass =

    arXiv

  184. [192]

    , keywords =

    Star Formation Efficiency in Nearby Galaxies Revealed with a New CO-to-H _ 2 Conversion Factor Prescription. , keywords =. doi:10.3847/1538-4357/ad10ae , archivePrefix =. 2310.16037 , primaryClass =

    arXiv

  185. [193]

    , keywords =

    The host of GRB 171205A in 3D: A resolved multiwavelength study of a rare grand-design spiral GRB host. , keywords =. doi:10.1051/0004-6361/202348141 , archivePrefix =. 2406.16725 , primaryClass =

    arXiv

  186. [194]

    The SN 2023ixf Progenitor in M101. II. Properties. , keywords =. doi:10.3847/1538-4357/ad414b , archivePrefix =. 2308.14844 , primaryClass =

    arXiv

  187. [195]

    , keywords =

    ALMA Reveals Spatially Resolved Properties of Molecular Gas in the Host Galaxy of FRB 20191001A at z = 0.2340. , keywords =. doi:10.3847/1538-4357/ad553f , archivePrefix =. 2407.01889 , primaryClass =

    arXiv

  188. [196]

    Science China Physics, Mechanics, and Astronomy , keywords =

    The dusty and extremely red progenitor of the type II supernova 2023ixf in Messier 101. Science China Physics, Mechanics, and Astronomy , keywords =. doi:10.1007/s11433-023-2267-0 , archivePrefix =. 2309.01389 , primaryClass =

    arXiv

  189. [197]

    , keywords =

    Filamentary Hierarchies and Superbubbles: Galactic Multiscale Magnetohydrodynamic Simulations of Giant Molecular Cloud to Star Cluster Formation. , keywords =. doi:10.3847/1538-4357/ad67e2 , archivePrefix =. 2405.18474 , primaryClass =

    arXiv

  190. [198]

    , keywords =

    Early light curve excess in Type IIb supernovae observed with ATLAS: Qualitative constraints on progenitor systems. , keywords =. doi:10.1051/0004-6361/202554370 , archivePrefix =. 2503.05909 , primaryClass =

  191. [199]

    , keywords =

    Star Formation from Low to High Mass: A Comparative View. , keywords =. doi:10.1146/annurev-astro-013125-122023 , archivePrefix =. 2501.16866 , primaryClass =

    arXiv

  192. [200]

    , keywords =

    Hydrodynamic Modelling of Early Peaks in Type Ibc Supernovae with Circumstellar Interaction. , keywords =. doi:10.1093/mnras/staf1382 , archivePrefix =. 2504.06445 , primaryClass =

    arXiv

  193. [201]

    , keywords =

    Constraining Resolved Extragalactic R _ 21 Variation with Well-calibrated ALMA Observations. , keywords =. doi:10.3847/1538-4357/addf4c , archivePrefix =. 2506.09125 , primaryClass =

    arXiv

  194. [202]

    , keywords =

    Laboratory Modeling of Supernova Remnants Collisions: Implications for Triggered Star Formation. , keywords =. doi:10.3847/1538-4357/ae2acf , archivePrefix =. 2508.05151 , primaryClass =

  195. [203]

    , keywords =

    Betelgeuse, Betelgeuse, Betelgeuse, Betel-buddy? Constraints on the Dynamical Companion to Orionis from HST. , keywords =. doi:10.3847/1538-4357/ae0c0c , archivePrefix =. 2505.18375 , primaryClass =

  196. [204]

    , keywords =

    The quest for blue supergiants: binary merger models for the evolution of the progenitor of SN 1987A. , keywords =. doi:10.3847/2041-8213/adeaaf , archivePrefix =. 2507.15749 , primaryClass =

    arXiv

  197. [205]

    , keywords =

    Dynamically Driven Evolution of Molecular Gas in the Barred Spiral Galaxy M83 Traced by CO J = 2─1/1─0 Line Ratio Variations. , keywords =. doi:10.3847/1538-4357/add1dc , adsurl =

    doi

  198. [206]

    arXiv e-prints , keywords =

    Revealing the Connection Between the Filamentary Hierarchy and Star Cluster Formation in a Simulated NGC 628 Galaxy. arXiv e-prints , keywords =. doi:10.48550/arXiv.2511.10486 , archivePrefix =. 2511.10486 , primaryClass =

    doi arXiv

  199. [207]

    , keywords =

    The Arizona Molecular ISM Survey with the SMT: Variations in the CO(2 1)/CO(1 0) Line Ratio across the Galaxy Population. , keywords =. doi:10.3847/1538-4357/ada361 , archivePrefix =. 2409.03963 , primaryClass =

    arXiv

  200. [208]

    arXiv e-prints , keywords =

    Cloud-scale gas properties, depletion times, and star formation efficiency per free-fall time in PHANGS--ALMA. arXiv e-prints , keywords =. doi:10.48550/arXiv.2502.04481 , archivePrefix =. 2502.04481 , primaryClass =

    doi

  201. [209]

    , keywords =

    Turbulence inference from CO spectral observations. , keywords =. doi:10.1093/mnras/staf1503 , archivePrefix =. 2509.04818 , primaryClass =

    arXiv

  202. [210]

    arXiv e-prints , keywords =

    Examining Turbulence in Galactic Molecular Clouds - II: Continuity of Turbulence Cascading in a Portion of the Local Arm. arXiv e-prints , keywords =. doi:10.48550/arXiv.2511.12418 , archivePrefix =. 2511.12418 , primaryClass =

    doi

  203. [211]

    Nature Astronomy , keywords =

    A high fraction of close massive binary stars at low metallicity. Nature Astronomy , keywords =. doi:10.1038/s41550-025-02610-x , archivePrefix =. 2509.12488 , primaryClass =

  204. [212]

    , keywords =

    The Observed Phase Space of Mass-loss History from Massive Stars Based on Radio Observations of a Large Supernova Sample. , keywords =. doi:10.3847/1538-4357/ad9e93 , adsurl =

    doi

  205. [213]

    , keywords =

    Binarity at LOw Metallicity (BLOeM): Enhanced multiplicity of early B-type dwarfs and giants at Z = 0.2 Z _. , keywords =. doi:10.1051/0004-6361/202453166 , archivePrefix =. 2503.21936 , primaryClass =

    arXiv

  206. [214]

    , keywords =

    Exclusion of a Direct Progenitor Detection for the Type Ic SN 2017ein Based on Late-time Observations. , keywords =. doi:10.3847/2041-8213/adad5d , archivePrefix =. 2411.17969 , primaryClass =

  207. [215]

    , keywords =

    The demographics of binary companions to stripped-envelope supernovae: confronting population synthesis models with observations. , keywords =. doi:10.1093/mnras/staf2208 , archivePrefix =. 2508.12677 , primaryClass =

  208. [216]

    , keywords =

    The Cold Molecular Gas Regulates the Activity of Active Galactic Nuclei in Massive Galaxies. , keywords =. doi:10.3847/1538-4357/ae4aa4 , archivePrefix =. 2603.27121 , primaryClass =

  209. [217]

    Digging into the Interior of Hot Cores with ALMA (DIHCA). VI. The Formation of Low-mass Multiple Systems in High-mass Cluster-forming Regions. , keywords =. doi:10.3847/1538-4357/ae371f , archivePrefix =. 2601.08904 , primaryClass =

  210. [218]

    arXiv e-prints , keywords =

    A binary merger product as the direct progenitor of a Type II-P supernova. arXiv e-prints , keywords =. doi:10.48550/arXiv.2601.06577 , archivePrefix =. 2601.06577 , primaryClass =

    doi

  211. [219]

    , keywords =

    The power of binaries on stripped-envelope supernovae across metallicity: uniform progenitor parameter space and persistently low ejecta masses, but subtype diversity. , keywords =. doi:10.1093/mnras/staf2163 , adsurl =

    doi

  212. [220]

    , year = 1939, month = may, volume =

    The Physical State of Interstellar Hydrogen. , year = 1939, month = may, volume =. doi:10.1086/144074 , adsurl =

    1939 doi

  213. [221]

    , year = 1973, month = nov, volume =

    Some Physical parameters of early-type stars. , year = 1973, month = nov, volume =. doi:10.1086/111498 , adsurl =

    1973 doi

  214. [222]

    , keywords =

    The Lyman-Continuum Fluxes and Stellar Parameters of O and Early B-Type Stars. , keywords =. doi:10.1086/177020 , adsurl =

    doi

  215. [223]

    , keywords =

    A new calibration of stellar parameters of Galactic O stars. , keywords =. doi:10.1051/0004-6361:20042386 , archivePrefix =. astro-ph/0503346 , primaryClass =

    arXiv

  216. [224]

    Astrophysics of gaseous nebulae and active galactic nuclei

  217. [225]

    , keywords =

    Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants. , keywords =. doi:10.1051/0004-6361/202449638 , archivePrefix =. 2402.11008 , primaryClass =

    arXiv

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Reviewed August 14, 2026 · model on record in the stance chip above.