On the Nature of Compact Galactic Nuclei

Details On the Nature of Compact Galactic Nuclei On the Nature of Compact Galactic Nuclei

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap.....41...24g&link_type=abstract

Astrophysics, Volume 41, Issue 1, pp.24-31

Astronomy and Astrophysics

Astrophysics

Scientific paper

Spherically symmetric stellar clusters (compact galactic nuclei and globular clusters), far advanced toward the state of complete statistical equilibrium in the course of evolution, are investigated. The equation of state of such systems (a polytrope with an index k = 0.5) is derived and their main characteristics are calculated. It is shown that compact galactic nuclei must consist mainly of rapidly rotating neutron stars and white dwarfs. It is demonstrated that pulsars may be created by the evaporation of neutron stars from the nucleus of our Galaxy. The number of such pulsars is ~3.106.

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