Dissipation of star clusters and the formation of coronas and moving clusters

Details Dissipation of star clusters and the formation of coronas and moving clusters Dissipation of star clusters and the formation of coronas and moving clusters

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979azh....56....9a&link_type=abstract

Astronomicheskii Zhurnal, vol. 56, no. 1, 1979, p. 9-15. In Russian.

Astronomy and Astrophysics

Astrophysics

9

Astrophysics, Galactic Evolution, Milky Way Galaxy, Star Clusters, Coronas, Galactic Structure, Gravitational Effects, Open Clusters, Star Distribution

Scientific paper

It is shown that a corona may be formed around star clusters by the irregular forces of the star field in which the clusters are embedded. This process is found to be effective only for open star clusters. An analysis is performed which indicates that some of the cluster stars will escape to the general star field and others will migrate to the corona when the central body in an open cluster disintegrates and that the cluster corona will be a moving cluster for a cosmogonically long time after complete disintegration of the central body. It is concluded that the Galactic disk is composed to a large extent of many interpenetrating moving clusters.

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