Gross Evolution of Spatial Distributions of Stars in Spherical Stellar Clusters

Details Gross Evolution of Spatial Distributions of Stars in Spherical Stellar Clusters Gross Evolution of Spatial Distributions of Stars in Spherical Stellar Clusters

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988atsir1528....9d&link_type=abstract

Astronomicheskii Tsirkulyar NO. 1528/MAY, P. 9, 1988

Astronomy and Astrophysics

Astronomy

1

Scientific paper

There exist three different ways of halo-core evolution under the effect
of irregular forces in quasistationary stellar systems. Both, damping
and increasing of regular field variations with time by different
velocities of the core-mass variation are possible in star clusters as a
result of core-halo stellar transitions.

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