Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-09-05
Mon.Not.Roy.Astron.Soc. 334 (2002) 310
Astronomy and Astrophysics
Astrophysics
12 pages (MNLaTeX), 17 Postscript figures, Submitted to MNRAS
Scientific paper
10.1046/j.1365-8711.2002.05420.x
We present the first post core collapse models of initially rotating star clusters, using the numerical solution of an orbit-averaged 2D Fokker-Planck equation. Based on the code developed by Einsel & Spurzem (1999), we have improved the speed and the stability and included the steady three-body binary heating source. We have confirmed that rotating clusters, whether they are in a tidal field or not, evolve significantly faster than non-rotating ones. Consequences for observed shapes, density distribution, and kinematic properties of young and old star clusters are discussed. The results are compared with gaseous and 1D Fokker-Planck models in the non-rotating case.
Einsel Christian
Kim Eunhyeuk
Lee Hyung Mok
Lee Myung Gyoon
Spurzem Rainer
No associations
LandOfFree
Dynamical evolution of rotating stellar systems - II. Post-collapse, equal mass system 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 Dynamical evolution of rotating stellar systems - II. Post-collapse, equal mass system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamical evolution of rotating stellar systems - II. Post-collapse, equal mass system will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-714883