Redshifts of ROSAT X-ray brightest clusters (Crawford+, 1995)

Details Redshifts of ROSAT X-ray brightest clusters (Crawford+, 1995) Redshifts of ROSAT X-ray brightest clusters (Crawford+, 1995)

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat..72740075c&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/274/75. Originally published in: 1995MNRAS.274...75C

Mathematics

Probability

Clusters: Galaxy, X-Ray Sources, Redshifts

Scientific paper

We report results from the second stage of an optical follow-up study aimed at determining new redshifts for clusters of galaxies selected from the ROSAT All-Sky Survey. We review the optical properties of all the clusters obtained so far in this programme, which comprises 71 clusters up to a redshift of 0.3. The fraction of central galaxies exhibiting optical line emission and an excess blue continuum is 34%, consistent with smaller, previous, X-ray samples. There is no trend for this fraction to increase with redshift, although we find a clear tendency for the strongest line emitters to have the bluest continua. The probability of the presence of line emission and an excess blue continuum is increased for those galaxies with associated radio sources, although the strength of these features does not appear to be related to the power of the radio emission.
(1 data file).

Affiliated with

Also associated with

No associations

Rating

Redshifts of ROSAT X-ray brightest clusters (Crawford+, 1995) 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 Redshifts of ROSAT X-ray brightest clusters (Crawford+, 1995), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Redshifts of ROSAT X-ray brightest clusters (Crawford+, 1995) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1666235