The evolution of a system of stars in an external environment

Details The evolution of a system of stars in an external environment The evolution of a system of stars in an external environment

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...364..100k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 364, Nov. 20, 1990, p. 100-103. Research supported by the Aspen Center for

Statistics

Computation

3

Globular Clusters, Stellar Evolution, Stellar Systems, Computational Astrophysics, Galactic Nuclei, Red Shift

Scientific paper

The homologous evolution of a stellar system losing stars and binding energy is analytically studied. How the evolution may be altered by allowing for a low-density environment of surrounding stars, from which the system can capture stars and/or energy, is addressed. The results indicate that, if the environment's influence is sufficiently strong, the system may cease to contract and actually begin to expand. The capture of stars and/or energy always decreases the value of the redshift for a given population.

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