Intense Star Cluster Formation: Stellar Masses, the Mass Function, and the Fundamental Mass Scale
Within the birth environment of a massive globular cluster, the combination of a luminous young stellar population and a high column density induces a state in which the thermal optical depth and radiation pressure are both appreciable. In this state, the sonic mass scale, which influences the peak...
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| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
IOP Publishing
2024-01-01
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| Serie: | The Astrophysical Journal Letters |
| Soggetti: | |
| Accesso online: | https://doi.org/10.3847/2041-8213/ad85d4 |
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