Stellar systems fed by outside stars - The evolution of model galactic nuclei

Details Stellar systems fed by outside stars - The evolution of model galactic nuclei Stellar systems fed by outside stars - The evolution of model galactic nuclei

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..335d&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, May 1985, p. 335-342) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, May-June

Astronomy and Astrophysics

Astronomy

Galactic Nuclei, Star Clusters, Stellar Evolution, Stellar Systems, Energy Distribution, Stellar Cores, Stellar Mass, Stellar Mass Ejection

Scientific paper

Extended rarefied environments around the core of a non-isothermic galactic nucleus can supply the core by both energies and masses of external stars due to relaxation mechanisms. These factors can influence considerably the secular evolution of the core when competing with usual star evaporation from it. Conditions are found under which external environments influence the core evolution much more than star evaporation. This results in expansion of the core instead of its collapse.

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