Spherically Symmetric Stellar Clusters with Anisotropy and Cutoff Energy in Momentum Distribution. II. The Relativistic Regime

Details Spherically Symmetric Stellar Clusters with Anisotropy and Cutoff Energy in Momentum Distribution. II. The Relativistic Regime Spherically Symmetric Stellar Clusters with Anisotropy and Cutoff Energy in Momentum Distribution. II. The Relativistic Regime

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010apj...709.1174b&link_type=abstract

The Astrophysical Journal, Volume 709, Issue 2, pp. 1174-1182 (2010).

Astronomy and Astrophysics

Astronomy

Dense Matter, Galaxies: Star Clusters: General, Hydrodynamics, Relativistic Processes

Scientific paper

We numerically construct models of spherically symmetric relativistic stellar clusters with anisotropic distribution functions. Newtonian solutions obtained in Paper I are generalized as isotropic Maxwellian ones with energy cutoff in their distribution function. We consider distributions with different levels of anisotropy and discuss some general characteristics of the models.

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