C1 1358 + 6245 at Z = 0.32 - an X-ray selected, distant, rich cluster of galaxies

Details C1 1358 + 6245 at Z = 0.32 - an X-ray selected, distant, rich cluster of galaxies C1 1358 + 6245 at Z = 0.32 - an X-ray selected, distant, rich cluster of galaxies

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aj....102....1l&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 102, July 1991, p. 1-13, 430.

Astronomy and Astrophysics

Astronomy

23

Astronomical Photometry, Galactic Clusters, X Ray Astronomy, Astronomical Spectroscopy, Color-Magnitude Diagram, Galactic Structure, Red Shift

Scientific paper

Results are presented from BVRI CCD photometric observations of C1 1358 + 6245, a distant cluster of galaxies. The spectrum of the optically dominant galaxy places the cluster at a redshift of z = 0.32. The C1 1358 + 6245 cluster is X-ray luminous, extremely rich (at least Abell Richness Class 3), contains a compact concentrated core of galaxies, and exhibits the Butcher-Oemler effect with a blue galaxy fraction between values 0.10 and 0.18. The brightest galaxy in the cluster has an absolute visual magnitude -22.89 and a rest frame color of (B-V)rf = 0.94.

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