Star cluster formation in a turbulent molecular cloud self-regulated by photoionization feedback

Abstract Most stars in the Galaxy are believed to be formed within star clusters from collapsing molecular clouds. However, the complete process of star formation, from the parent cloud to a gas-free star cluster, is still poorly understood. We perform radiation-hydrodynamical simulations of the col...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2017-12, Vol.472 (4), p.4155-4172
Hauptverfasser: Gavagnin, Elena, Bleuler, Andreas, Rosdahl, Joakim, Teyssier, Romain
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Sprache:eng
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