Stability of dense stellar clusters against relativistic collapse. II. Maxwellian distribution functions with different cutoff parameters

Astrophysical Journal

Volumn 500, Issue 1 PART I, 1998, Pages 217-232

  Bisnovatyi Kogan, G S ^a   Merafina, M ^b   Ruffini, R ^c   Vesperini, E ^d  

^a ICRANET   (Italy)

^b Space Research Institute ^*  (Russian Federation)

^c SAPIENZA UNIVERSITY OF ROME   (Italy)

^d SCUOLA NORMALE SUPERIORE   (Italy)

Author keywords

Celestial mechanics, stellar dynamics; Globular clusters: General; Relativity

Indexed keywords

EID: 22044448429     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/305689     Document Type: Article

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