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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Autors principals:	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
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2026-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	Interstellar medium Stellar feedback Massive stars Supernovae Radio astronomy Millimeter astronomy
Accés en línia:	https://doi.org/10.3847/1538-4357/ae3f33
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