Instabilities in inhomogeneous collision-free self-gravitating stellar systems

Details Instabilities in inhomogeneous collision-free self-gravitating stellar systems Instabilities in inhomogeneous collision-free self-gravitating stellar systems

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981plap.rept..385s&link_type=abstract

In ESA Plasma Astrophys. p 385-389 (SEE N82-20030 10-88)

Statistics

Applications

Astrodynamics, Dynamic Stability, Elliptical Galaxies, Star Distribution, Stellar Gravitation, Stellar Systems, Collisionless Plasmas, Equilibrium Equations, Kinetic Theory, Symmetry

Scientific paper

Stability criteria for collision-free self-gravitating stellar systems
are discussed with applications to elliptical galaxies. It is concluded
that rotationally symmetric systems which are either sufficiently oblate
or prolate are unstable against ringlike and sausagelike perturbations,
respectively.

Affiliated with

Also associated with

No associations

Rating

Instabilities in inhomogeneous collision-free self-gravitating stellar systems 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 Instabilities in inhomogeneous collision-free self-gravitating stellar systems, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Instabilities in inhomogeneous collision-free self-gravitating stellar systems will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-744858