Ellipsoidal self-consistent phase models of stellar systems

Details Ellipsoidal self-consistent phase models of stellar systems Ellipsoidal self-consistent phase models of stellar systems

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.274..657k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 274, Issue 3, pp. 657-669.

Astronomy and Astrophysics

Astronomy

Hydrodynamics, Methods: Analytical, Celestial Mechanics, Stellar Dynamics

Scientific paper

This paper presents a review of the dynamics of collisionless, homogeneous gravitating ellipsoids. A combined method for the construction of self-consistent models is applied, which takes into account both the elements of the kinetic method and those of the hydrodynamical description. We study both non-stationary models and equilibrium figures. An intrinsic characteristic of these models is that they are all, in one way or another, degenerate in six-dimensional phase ellipsoids.

Affiliated with

Also associated with

No associations

Rating

Ellipsoidal self-consistent phase models of 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 Ellipsoidal self-consistent phase models of stellar systems, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ellipsoidal self-consistent phase models of stellar systems will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-755783