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The Hierarchical Dynamical State of Molecular Gas from 3 to 300 pc in NGC 253

Understanding how the dynamical state of the interstellar medium (ISM) changes across spatial scales can provide important insights into how the gas is organized and ultimately collapses to form stars. To this end, we present ALMA ^12 CO(2–1) observations at 7 pc (0 $\mathop{.}\limits^{\unicode{x020...

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Autores principales: Elias K. Oakes, Christopher M. Faesi, Erik Rosolowsky, Adam K. Leroy, Simon C. O. Glover, Annie Hughes, Sharon E. Meidt, Eva Schinnerer, Jiayi Sun, Amirnezam Amiri, Ashley T. Barnes, Zein Bazzi, Ivana Bešlić, Frank Bigiel, Guillermo A. Blanc, Charlie Burton, Ryan Chown, Enrico Congiu, Daniel A. Dale, Simthembile Dlamini, Hao He, Eric W. Koch, Fu-Heng Liang, Jérôme Pety, Miguel Querejeta, Sumit K. Sarbadhicary, Sophia K. Stuber, Antonio Usero, Thomas G. Williams
Formato: Artigo
Lenguaje:Inglês
Publicado: IOP Publishing 2025-01-01
Colección:The Astrophysical Journal
Materias:
Interstellar medium
Giant molecular clouds
Molecular gas
Star formation
Starburst galaxies
Acceso en línea:https://doi.org/10.3847/1538-4357/ae0642
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