CO depletion in infrared dark clouds
Context. Infrared dark clouds (IRDCs) are cold, dense structures that are likely representative of the initial conditions of star formation. Many studies of IRDCs employ CO to investigate cloud dynamics, but CO can be highly depleted from the gas phase in IRDCs, which affects its fidelity as tracer....
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| Autors principals: | , , , , , , , , , , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
EDP Sciences
2026-01-01
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| Col·lecció: | Astronomy & Astrophysics |
| Matèries: | |
| Accés en línia: | https://www.aanda.org/articles/aa/full_html/2026/01/aa57102-25/aa57102-25.html |
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