Formation of hierarchical multiple protostellar cores

Details Formation of hierarchical multiple protostellar cores Formation of hierarchical multiple protostellar cores

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991natur.351..298b&link_type=abstract

Nature (ISSN 0028-0836), vol. 351, May 23, 1991, p. 298-300.

Physics

63

Binary Stars, Protostars, Star Formation, Stellar Cores, Stellar Evolution, Triple Stars, Conservation Laws, Gravitational Collapse, Magnetohydrodynamics, Pre-Main Sequence Stars, Stellar Models

Scientific paper

Numerical hydrodynamical calculations are described which show that stable hierarchical systems of multiple protostellar cores can form through gravitationally driven fragmentation during the collapse of an isolated gas cloud. The results suggest that the hierarchical systems observed may be the result of the hydrodynamical collapse of rapidly rotating clouds.

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