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Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster

Ralf S. Klessen·Andreas Burkert
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Abstract

Using smoothed particle hydrodynamics in combination with the special-purpose hardware device GRAPE, we follow the fragmentation process and dynamical evolution in the interior of molecular clouds until most of the gas is converted to form a cluster of protostellar cores. The properties of this protostellar cluster are compared to observational data from star forming regions.

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Ralf S. Klessen, Andreas Burkert. 1997-10-28. Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster. https://arxiv.org/abs/astro-ph/9710318

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