Stability of self-gravitating spherical systems in which phase space density is a function of energy and angular momentum, for spherical perturbations

Details Stability of self-gravitating spherical systems in which phase space density is a function of energy and angular momentum, for spherical perturbations Stability of self-gravitating spherical systems in which phase space density is a function of energy and angular momentum, for spherical perturbations

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....50..467g&link_type=abstract

Astronomy and Astrophysics, vol. 50, no. 3, Aug. 1976, p. 467-470.

Astronomy and Astrophysics

Astrophysics

14

Angular Momentum, Perturbation Theory, Star Clusters, Star Distribution, Astronomical Models, Distribution Functions, Poisson Equation, Spheres, Steady State, Vlasov Equations

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1976A&A....50..467G

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