Numerical simulations of open clusters

Details Numerical simulations of open clusters Numerical simulations of open clusters

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40..283o&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Open Clusters And Associations: Individual (Ngc 6475), Methods: Numerical

Scientific paper

We performed N-body numerical simulations of NGC 6475, using its observed stellar positions, proper motions and momenta of the radial velocity distribution as initial conditions. Also, we statistically recovered stellar positions and velocities with respect to the plane of the sky. We found the system is highly unstable, probably due to an excess of positive energy.

Affiliated with

Also associated with

No associations

Rating

Numerical simulations of open 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 Numerical simulations of open clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical simulations of open clusters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1674544