Evolution of dense star clusters

Details Evolution of dense star clusters Evolution of dense star clusters

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pazh....4..130b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 4, Mar. 1978, p. 130-133.) Soviet Astronomy Letters, vol. 4, Mar.-Apr. 1978, p. 69-71.

Astronomy and Astrophysics

Astronomy

7

Star Clusters, Star Distribution, Stellar Evolution, Active Galactic Nuclei, Binary Stars, Black Holes (Astronomy), Celestial Mechanics, Collision Parameters, Globular Clusters, Gravitational Collapse, Quasars, Relativistic Effects, Stellar Mass Accretion, Velocity Distribution

Scientific paper

Evolutionary tracks are calculated and plotted for dense star clusters of various types, corresponding to globular clusters, active galactic nuclei, nuclear regions of elliptical galaxies, and quasars. Evaporation of stars from a cluster and head-on collisions between stars are taken into account. The evolution of the clusters is described qualitatively and traced to the point where relativistic collapse or cluster breakup occurs. Effects of binary formation in clusters with a small number of members are briefly examined, along with effects of black-hole formation due to accretion.

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