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Where Do Stars Explode in the ISM?—The Distribution of Dense Gas around Evolved Massive Stars in M33

The effect of supernovae (SNe) on star formation in the interstellar medium (ISM) depends sensitively on where SNe explode with respect to ISM clouds. Observationally, SN ISM environments characterized by spatially resolved gas maps can empirically guide the placement of SNe in subgrid models, but u...

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Asıl Yazarlar: Sumit K. Sarbadhicary, Jordan Wagner, Eric W. Koch, Ness Mayker Chen, Adam K. Leroy, Natalia Lahén, Erik Rosolowsky, Kathryn F. Neugent, Chang-Goo Kim, Laura Chomiuk, Julianne J. Dalcanton, Laura A. Lopez, Nickolas M. Pingel, Remy Indebetouw, Thomas G. Williams, Elizabeth Tarantino, Jennifer Donovan Meyer, Evan D. Skillman, Adam Smercina, Amanda A. Kepley, Eric J. Murphy, Jay Strader, Tony Wong, Snežana Stanimirović, Vicente Villanueva, Fabian Walter, Juergen Ott, Jeremy Darling, Julia Roman-Duval, Claire E. Murray
Materyal Türü: Artigo
Dil:Inglês
Baskı/Yayın Bilgisi: IOP Publishing 2026-01-01
Seri Bilgileri:The Astrophysical Journal
Konular:
Interstellar medium
Stellar feedback
Massive stars
Supernovae
Radio astronomy
Millimeter astronomy
Online Erişim:https://doi.org/10.3847/1538-4357/ae3f33
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