Star clusters containing massive, central black holes. III - Evolution calculations

Details Star clusters containing massive, central black holes. III - Evolution calculations Star clusters containing massive, central black holes. III - Evolution calculations

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...239..685m&link_type=abstract

Astrophysical Journal, Part 1, vol. 239, July 15, 1980, p. 685-704.

Astronomy and Astrophysics

Astronomy

79

Black Holes (Astronomy), Evolution (Development), Star Clusters, Star Distribution, Stellar Evolution, Astronomical Models, Computerized Simulation, Globular Clusters, Gravitational Collapse, Monte Carlo Method

Scientific paper

Two-dimensional simulations of the time evolution of a star cluster around a massive, central black hole are presented. A Monte-Carlo simulation scheme modified to provide time-dependent results is utilized. The simulations show that even a relatively small central black hole can halt core collapse and indicate that the cluster can achieve a quasi-static postcollapse configuration.

Affiliated with

Also associated with

No associations

Rating

Star clusters containing massive, central black holes. III - Evolution calculations 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 Star clusters containing massive, central black holes. III - Evolution calculations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Star clusters containing massive, central black holes. III - Evolution calculations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-803469