Molecular cloud dispersal traced by the ionized carbon 158 μm line

Feedback from massive stars in the form of radiation and winds impacts the associated host molecular cloud. Not only can feedback compress gas and trigger the formation of dense cores that eventually collapse into new stars, it can also disperse cloud material and lead to the destruction of the clou...

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Bibliografiske detaljer

Principais autores:	Bonne L., Schneider N., Dannhauer S., Keilmann E., Jackson J. M., Simon R., Tielens A. G. G. M., Chambers E., Buchbender C., Verbena J. L., Kabanovic S., Faerber T., Anderson L. D., Güsten R., Jacob A. M., Guevara C., Wyrowski F.
Format:	Artigo
Sprog:	Inglês
Udgivet:	EDP Sciences 2026-07-01
Serier:	Astronomy & Astrophysics
Fag:	ism: bubbles ism: clouds hii regions ism: kinematics and dynamics ism: molecules ism: structure
Online adgang:	https://www.aanda.org/articles/aa/full_html/2026/07/aa59930-26/aa59930-26.html
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