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, Marco
Writing – Original Draft Preparation
;
RUFFINI, Remo
Writing – 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.
1993
stellar clusters; relativistic collapse; dense matter
01 Pubblicazione su rivista::01a Articolo in rivista
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.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/67940
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