The velocity dispersion of the Corona Borealis cluster of galaxies

Details The velocity dispersion of the Corona Borealis cluster of galaxies The velocity dispersion of the Corona Borealis cluster of galaxies

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pasp...89..116s&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 89, Apr.-May 1977, p. 116-118.

Astronomy and Astrophysics

Astronomy

15

Galactic Clusters, Red Shift, X Ray Sources, Absorption Spectra, Astronomical Photography, Radial Velocity

Scientific paper

Redshifts were measured for eight relatively faint members of the Cor Bor cluster (A 2065). By combining these data with those of Humason et al., (1956), it is found that this rich cluster has a (relativistically corrected) velocity dispersion of 1070 km/s. This value is close to that found for the Coma cluster, and thus A 2065 should be a detectable extended X-ray source in future deep X-ray surveys.

Affiliated with

Also associated with

No associations

Rating

The velocity dispersion of the Corona Borealis cluster of galaxies 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 The velocity dispersion of the Corona Borealis cluster of galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The velocity dispersion of the Corona Borealis cluster of galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1618566