Star Cluster Formation in a Turbulent Molecular Cloud Self-Regulated by Photo-Ionisation Feedback

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 collapse of...

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Veröffentlicht in:	arXiv.org 2017-10
Hauptverfasser:	Gavagnin, Elena, Bleuler, Andreas, Rosdahl, Joakim, Teyssier, Romain
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Computer simulation Density Expulsion Feedback Galaxies High energy astronomy Ionization Ionizing radiation Molecular clouds Physics - Astrophysics of Galaxies Physics - Solar and Stellar Astrophysics Star & galaxy formation Star clusters Star formation Stellar mass
Online-Zugang:	Volltext
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