We numerically construct models of spherically symmetric relativistic stellar clusters with anisotropic distribution functions. Newtonian solutions obtained in Paper I are generalized as isotropicMaxwellian ones with energy cutoff in their distribution function.We consider distributions with different levels of anisotropy and discuss some general characteristics of the models.
SPHERICALLY SYMMETRIC STELLAR CLUSTERS WITH ANISOTROPY AND CUTOFF ENERGY IN MOMENTUM DISTRIBUTION. II. THE RELATIVISTIC REGIME / Gennady S., Bisnovatyi Kogan; Merafina, Marco; Maria Rosaria, Vaccarelli. - In: THE ASTROPHYSICAL JOURNAL. - ISSN 0004-637X. - ELETTRONICO. - 709:2(2010), pp. 1174-1182. [10.1088/0004-637x/709/2/1174]
SPHERICALLY SYMMETRIC STELLAR CLUSTERS WITH ANISOTROPY AND CUTOFF ENERGY IN MOMENTUM DISTRIBUTION. II. THE RELATIVISTIC REGIME
MERAFINA, Marco;
2010
Abstract
We numerically construct models of spherically symmetric relativistic stellar clusters with anisotropic distribution functions. Newtonian solutions obtained in Paper I are generalized as isotropicMaxwellian ones with energy cutoff in their distribution function.We consider distributions with different levels of anisotropy and discuss some general characteristics of the models.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.