Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...500..217b&link_type=abstract
Astrophysical Journal v.500, p.217
Astronomy and Astrophysics
Astronomy
5
Celestial Mechanics, Stellar Dynamics, Galaxy: Globular Clusters: General, Relativity
Scientific paper
We investigate the stability of dense stellar clusters against relativistic collapse by approximate methods described in the previous paper in this series. These methods, together with the analysis of the fractional binding energy of the system, have been applied to sequences of equilibrium models, with cutoff in the distribution function, which generalize those studied by Zeldovich & Podurets. We show the existence of extreme configurations, which are stable all the way up to infinite values of the central redshift.
Bisnovatyi-Kogan Gennadi S.
Merafina Marco
Ruffini Remo
Vesperini Enrico
No associations
LandOfFree
Stability of Dense Stellar Clusters against Relativistic Collapse. II. Maxwellian Distribution Functions with Different Cutoff Parameters does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Stability of Dense Stellar Clusters against Relativistic Collapse. II. Maxwellian Distribution Functions with Different Cutoff Parameters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stability of Dense Stellar Clusters against Relativistic Collapse. II. Maxwellian Distribution Functions with Different Cutoff Parameters will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1331264