Studies of radial velocity members for eight rich galaxy clusters.

Details Studies of radial velocity members for eight rich galaxy clusters. Studies of radial velocity members for eight rich galaxy clusters.

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996acaps..16..129s&link_type=abstract

Acta Astrophys. Sin., Vol. 16, No. 2, p. 129 - 136

Astronomy and Astrophysics

Astrophysics

Clusters Of Galaxies: Membership, Clusters Of Galaxies: Radial Velocities

Scientific paper

On the basis of a radial velocity membership determination method while the distribution of surface-number-density of galaxies in cluster regions is concerned simultaneously, the authors calculate the distribution parameters and membership probabilities of individual galaxies for 8 Abell clusters. Elongate structures seem to be a universal appearance for rich galaxy clusters. From these 8 clusters, they have found an obvious relationship between NA and σc of galaxy clusters, and furthermore, inferred that the mass to luminosity ratio of rich galaxy clusters are from 100 h100-1 to 600 h100-1, with the average value being 350 h100-1.

Affiliated with

Also associated with

No associations

Rating

Studies of radial velocity members for eight rich galaxy 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 Studies of radial velocity members for eight rich galaxy clusters., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Studies of radial velocity members for eight rich galaxy clusters. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1333007