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

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dc.creatorKlessen, Ralf S.
dc.creatorBurkert, Andreas
dc.date1997-10-28
dc.date.accessioned2026-07-07T02:24:50Z
dc.date.available2026-07-07T02:24:50Z
dc.descriptionUsing 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.
dc.description4 pages including three figures, LaTeX, to appear in the proceedings to the Riken Symposium on Supercomputing, held September 1 --3 1997 in Tokyo, (resolution of fig. 1 has been degraded to fit size requirements)
dc.identifierhttps://arxiv.org/abs/astro-ph/9710318
dc.identifierhttp://arxiv.org/abs/astro-ph/9710318
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11709
dc.subjectAstrophysics
dc.titleFragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster
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