Instability of rotating stellar systems with elongated orbits

Details Instability of rotating stellar systems with elongated orbits Instability of rotating stellar systems with elongated orbits

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18..431p&link_type=abstract

Soviet Astronomy Letters, Vol. 18, p. 431; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 12, p. 1052-1058. I

Statistics

Computation

Elliptical Galaxies, Galactic Bulge, Gravitational Effects, Stellar Orbits, Stellar Systems, Systems Stability, Computational Astrophysics, Disk Galaxies, Orbital Mechanics, Perturbation Theory

Scientific paper

The effect of rotation on the instability of radial orbits in collisionless gravitating systems (elliptical galaxies, bulges of disk galaxies, etc.) is examined. The dispersion relationship for the exactly solved problem of small perturbations in the simplest model of a rotating spherical cluster with highly elongated stellar orbits is derived and investigated.

Affiliated with

Also associated with

No associations

Rating

Instability of rotating stellar systems with elongated orbits does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Instability of rotating stellar systems with elongated orbits, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Instability of rotating stellar systems with elongated orbits will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1144218