Dynamical evolution of clusters with stellar mass loss

Details Dynamical evolution of clusters with stellar mass loss Dynamical evolution of clusters with stellar mass loss

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....58..363a&link_type=abstract

(European Workshop on White Dwarfs, 2nd, Rome, Italy, Sept. 1976.) Astronomy and Astrophysics, vol. 58, no. 3, June 1977, p. 363

Astronomy and Astrophysics

Astrophysics

18

Mass Transfer, Star Clusters, Stellar Evolution, Stellar Mass Ejection, White Dwarf Stars, Density (Number/Volume), Galactic Nuclei, Globular Clusters, Radial Velocity, Star Distribution, Stellar Models

Scientific paper

The dynamic evolution of large star clusters with two and three stellar groups (of initial masses between 0.1 and 2 solar masses) was investigated, the formation of white dwarfs being determined on the basis of the theory of evolution of single stars. It was found that stellar mass ejection has a considerable effect on the dynamic evolution of clusters by slowing down their rates of evolution and by preventing the formation of dense cores. It also has an effect on projected star densities, velocity dispersions, the distribution of light across the cluster, and synthetic lights and colors.

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