Stability of dense stellar clusters to relativistic collapse is investigated by an approximate method, similar to static criteria of stellar stability. The equilibrium models with Maxwellian distribution function with cutoff, studied by Zel'dovich and Podurets (ZP), have been considered.
Stability of the dense stellar clusters - II / BISNOVATYI KOGAN, G. S.; Merafina, Marco; Ruffini, Remo; Vesperini, E.. - In: PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC. - ISSN 0004-6280. - STAMPA. - 50:(1993), pp. 125-126.
Stability of the dense stellar clusters - II
MERAFINA, MarcoWriting – Original Draft Preparation
;RUFFINI, RemoWriting – Original Draft Preparation
;
1993
Abstract
Stability of dense stellar clusters to relativistic collapse is investigated by an approximate method, similar to static criteria of stellar stability. The equilibrium models with Maxwellian distribution function with cutoff, studied by Zel'dovich and Podurets (ZP), have been considered.File allegati a questo prodotto
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