Cool Dark Gas in Cygnus X: The First Large-scale Mapping of Low-frequency Carbon Recombination Lines

Understanding the transition from atomic gas to molecular gas is critical to explain the formation and evolution of molecular clouds. However, the gas phases involved, cold H i and CO-dark molecular gas, are challenging to directly observe and physically characterize. We observed the Cygnus X star-f...

Πλήρης περιγραφή

Λεπτομέρειες βιβλιογραφικής εγγραφής

Κύριοι συγγραφείς:	Kimberly L. Emig, Pedro Salas, Loren D. Anderson, D. Anish Roshi, Lars Bonne, Alberto D. Bolatto, Isabelle A. Grenier, Rebecca C. Levy, Dylan J. Linville, Matteo Luisi, M. Riley Owens, J. Poojapriyatharsheni, Nicola Schneider, Luigi Tibaldo, Alexander G. G. M. Tielens, Stefanie K. Walch, Glenn J. White
Μορφή:	Artigo
Γλώσσα:	Inglês
Έκδοση:	IOP Publishing 2025-01-01
Σειρά:	The Astrophysical Journal
Θέματα:	Interstellar medium Interstellar clouds Interstellar atomic gas Radio spectroscopy the Milky Way
Διαθέσιμο Online:	https://doi.org/10.3847/1538-4357/adfa17
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