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....
I tiakina i:
| Ngā kaituhi matua: | , , , , , , , , , , , , |
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| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
EDP Sciences
2026-01-01
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| Rangatū: | Astronomy & Astrophysics |
| Ngā marau: | |
| Urunga tuihono: | https://www.aanda.org/articles/aa/full_html/2026/01/aa57102-25/aa57102-25.html |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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