Estimates of Relaxation Times in Numerical Dynamical Models of Open Star Clusters

Details Estimates of Relaxation Times in Numerical Dynamical Models of Open Star Clusters Estimates of Relaxation Times in Numerical Dynamical Models of Open Star Clusters

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003arep...47..483d&link_type=abstract

Astronomy Reports, vol. 47, Issue 6, p.483-491

Astronomy and Astrophysics

Astronomy

Scientific paper

Relaxation times in the spaces of several stellar-motion parameters are obtained for a number of open-cluster models. The differences between the relaxation times in these spaces increase with the degree of nonstationarity of the cluster models. In the course of the cluster’s evolution, the relaxation times increase in all the spaces considered. During violent relaxation, the stars occupy all domains accessible to them, first in absolute velocity and then in clustercentric distance. The dependence of the coarse-grained phase-space density of the cluster on small initial perturbations of the phase-space coordinates of its constituent stars tends to decrease at times exceeding the time scales for violent and “collisional” relaxation.

Affiliated with

Also associated with

No associations

Rating

Estimates of Relaxation Times in Numerical Dynamical Models of Open Star 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 Estimates of Relaxation Times in Numerical Dynamical Models of Open Star Clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Estimates of Relaxation Times in Numerical Dynamical Models of Open Star Clusters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1820715