The formation of a gaseous and stellar disk structure in a dense stellar cluster

Details The formation of a gaseous and stellar disk structure in a dense stellar cluster The formation of a gaseous and stellar disk structure in a dense stellar cluster

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65..290i&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Mar.-Apr. 1988, p. 290-299. In Russian.

Physics

3

Protostars, Star Clusters, Star Formation, Stellar Physics, Galactic Nuclei, Inelastic Collisions, Milky Way Galaxy, Stellar Mass

Scientific paper

The conditions of star formation process in dense star clusters,
undergoing inelastic contact collisions, are investigated. The gas
released in collisions is shown to contract to a cold disc with a
temperature of ≡102- 103K, where mainly
low-mass stars ≡0.1 - 0.5 M_sun; are formed.

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