Post-collapse evolution of small-N clusters

Details Post-collapse evolution of small-N clusters Post-collapse evolution of small-N clusters

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.118..367i&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Statistics

Computation

1

Fokker-Planck Equation, Globular Clusters, Gravitational Collapse, Many Body Problem, Stellar Evolution, Binary Stars, Computational Astrophysics, Stellar Mass

Scientific paper

N-body simulations were made to study post-collapse evolution of small-N
clusters. The qualitative behaviour of the dynamical evolution is the
same as in the Fokker-Planck approximation. The flatter the mass
spectrum is the more violent is the activity of binaries and so are the
expansion and contraction of the cluster core.

Affiliated with

Also associated with

No associations

Rating

Post-collapse evolution of small-N clusters 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 Post-collapse evolution of small-N clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Post-collapse evolution of small-N clusters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1844143