Catastrophe theory and stellar systems

Details Catastrophe theory and stellar systems Catastrophe theory and stellar systems

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....26..139g&link_type=abstract

(Astrofizika, vol. 26, Jan.-Feb. 1987, p. 139-151) Astrophysics (ISSN 0571-7132), vol. 26, no. 1, July 1987, p. 82-90. Translati

Statistics

Computation

Catastrophe Theory, Computational Astrophysics, Stellar Systems, Black Holes (Astronomy), Dynamical Systems, High Temperature

Scientific paper

The manifestation of a gravothermal catastrophe for a stellar system containing a massive central body is examined from the point of view of catastrophe theory. It is shown that the catastrophe of A2 type that holds for a system without a massive center persists in this case too and does not become a cusp. The catastrophe occurs at higher temperatures of the system and lower values of the density contrast.

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