Internal kinematics of open star clusters

Details Internal kinematics of open star clusters Internal kinematics of open star clusters

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.236..865s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 236, Feb. 15, 1989, p. 865-874.

Astronomy and Astrophysics

Astronomy

10

Kinematics, Star Clusters, Stellar Motions, Anisotropy, Stellar Mass, Velocity Distribution

Scientific paper

Proper motion measurements are employed to investigate the internal
kinematics of eight open star clusters. In most of the clusters
considered, no dependence of the intrinsic dispersion in proper motion
on stellar mass and radial distance from the cluster center is noted.
Velocity isotropy is found in all of the clusters except NGC 2516.

Affiliated with

Also associated with

No associations

Rating

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

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1885312