The stability of a differentially rotating disk of stars

Details The stability of a differentially rotating disk of stars The stability of a differentially rotating disk of stars

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982azh....59.1081c&link_type=abstract

(Astronomicheskii Zhurnal, vol. 59, Nov.-Dec. 1982, p. 1081-1088) Soviet Astronomy (ISSN 0038-5301), vol. 26, Nov.-Dec. 1982, p.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Disk Galaxies, Galactic Rotation, Star Distribution, Equilibrium Equations, Gravitational Fields, Perturbation Theory

Scientific paper

The problem of whether certain models of infinitely thin, differentially
rotating disks of stars will be stable against double-arm spiral
disturbances is solved. Both the differential rotation and the spherical
component of the galaxy wil serve to stabilize the bar mode.

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