On the stability of a gaseous disk embedded in a stellar system

Details On the stability of a gaseous disk embedded in a stellar system On the stability of a gaseous disk embedded in a stellar system

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60..257a&link_type=abstract

(Astronomicheskii Zhurnal, vol. 60, Mar.-Apr. 1983, p. 257-261) Soviet Astronomy (ISSN 0038-5301), vol. 27, Mar.-Apr. 1983, p. 1

Astronomy and Astrophysics

Astronomy

Galactic Structure, Interstellar Gas, Rotating Matter, Star Distribution, Systems Stability, Density Distribution, Gas Density, Gravitational Fields, Propagation Modes

Scientific paper

A theoretical investigation of the stability of a rotating, finite-radius gas disk embedded in a spheroidal stellar system is presented, extending the analysis of Abramyan and Kaplan (1976), Kaplan et al. (1977) and Abramyan and Oganesyan (1978). The results are presented in graphic, tabular, and equation form and discussed. The gravitational field of the stellar system is shown to be unable to fully damp the instability of a slowly rotating disk, although it should facilitate disk stabilization.

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