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...

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Veröffentlicht in:	Astrophysical journal. Letters 2023-02, Vol.944 (2), p.L32
Hauptverfasser:	Silich, Sergiy, Turner, Jean, Mackey, Jonathan, Martínez-González, Sergio
Format:	Artikel
Sprache:	eng
Schlagworte:	Clouds Density distribution Dwarf galaxies Energy dissipation Galaxies Gas density Massive stars Molecular gases Residual gas Spheroidal galaxies Star & galaxy formation Star clusters Star formation Turbulent energy Wind
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