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...
| Published in: | The Astrophysical Journal Letters |
|---|---|
| Main Authors: | , , , |
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2023-01-01
|
| Subjects: | |
| Online Access: | https://doi.org/10.3847/2041-8213/acb687 |