Dense Gas Properties and Star Formation in M82
High-density molecular gas plays a vital role in supporting star formation within galaxies. However, traditional tracers of dense gas, such as the low- J transitions of HCN and HCO ^+ , are predominantly optically thick. This characteristic presents a significant challenge in accurately estimating t...
Guardat en:
| Autors principals: | , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
IOP Publishing
2025-01-01
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| Col·lecció: | The Astrophysical Journal |
| Matèries: | |
| Accés en línia: | https://doi.org/10.3847/1538-4357/ae0038 |
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