High resolution kinematics of galactic globular clusters.

Details High resolution kinematics of galactic globular clusters. High resolution kinematics of galactic globular clusters.

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...258..302z&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 258, no. 2, p. 302-308.

Astronomy and Astrophysics

Astrophysics

20

Globular Clusters, Gravitational Collapse, Kinematics, Mass To Light Ratios, Stellar Cores, High Resolution, Radial Velocity, Star Formation, Stellar Evolution

Scientific paper

We present integrated central velocity dispersions for 7 globular clusters, three of which known to be post core-collapsed. Discussion of the statistical significance of the measurements is presented. For one of the clusters, M30, we also provide radial velocities of 16 stars, which help mapping the inner velocity dispersion profile. Our data suggest that M30 has more likely an isothermal core, at variance with the behavior of its closest twin M15.

Affiliated with

Also associated with

No associations

Rating

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

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1512015