The dynamics of forming open stellar clusters

Details The dynamics of forming open stellar clusters The dynamics of forming open stellar clusters

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64..656d&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, May-June 1987, p. 656-659. In Russian.

Astronomy and Astrophysics

Astronomy

1

Astrodynamics, Molecular Clouds, Open Clusters, Star Formation, Stellar Evolution, Stellar Models, B Stars, Binary Stars, O Stars, Stellar Gravitation

Scientific paper

The formation of bound open stellar-clusters (BOSC) in the cores of molecular clouds with low 'global' star-formation efficiency is considered. Due to the impulsive loss of gas from the system, a BOSC can be formed if the radius of the tidally stable molecular clouds is five times greater than that of the BOSC. It is noted that the 'impulsive' loss of these gas masses changes the BOSC potential, but alters the strong field of the cluster only slightly.

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