Theory of the stability of flat subsystems of galaxies

Details Theory of the stability of flat subsystems of galaxies Theory of the stability of flat subsystems of galaxies

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982afz....18..350a&link_type=abstract

(Astrofizika, vol. 18, July-Sept. 1982, p. 350-355) Astrophysics (ISSN 0571-7132), vol. 18, no. 3, Jan. 1983, p. 213-216. Transl

Astronomy and Astrophysics

Astrophysics

1

Galactic Structure, Halos, Interstellar Gas, Mass Distribution, Polytropic Processes, Stellar Gravitation, Gas Density, Milky Way Galaxy, Stability, Star Distribution

Scientific paper

The stability criterions of polytropic (γ = 2) and homogeneous
layers are obtained, taking into account the gravitation of the
spheroidal halo. The critical mass values of the halo stabilizing the
input flat subsystem are estimated.

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