Molecular Gas Properties in Young Stellar Clusters with a Suppressed Star Cluster Wind
In compact and dense star-forming clouds a global star cluster wind could be suppressed. In this case stellar feedback is unable to expel the leftover gas from the cluster. Young massive stars remain embedded in a dense residual gas and stir it by moving in the gravitational well of the system. Here...
Wedi'i Gadw mewn:
| Prif Awduron: | , , , |
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| Fformat: | Artigo |
| Iaith: | Inglês |
| Cyhoeddwyd: |
IOP Publishing
2023-01-01
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| Cyfres: | The Astrophysical Journal Letters |
| Pynciau: | |
| Mynediad Ar-lein: | https://doi.org/10.3847/2041-8213/acb687 |
| Tagiau: |
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