CCD observations of a rich distant cluster of galaxies (1046 = 35) containing a classical double radio source

Details CCD observations of a rich distant cluster of galaxies (1046 = 35) containing a classical double radio source CCD observations of a rich distant cluster of galaxies (1046 = 35) containing a classical double radio source

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.214...27e&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 214, May 1, 1985, p. 27-32. Research supported by the S

Astronomy and Astrophysics

Astronomy

6

Astronomical Spectroscopy, Charge Coupled Devices, Galactic Clusters, Radio Sources (Astronomy), Data Processing, Red Shift

Scientific paper

CCD imaging observations conducted with the Kitt Peak 0.9-m telescope have revealed a cluster of galaxies at RA 10 h 46 m 03 s, Dec 35 deg 47 min 28 sec (1950.0). The cluster, which is of richness class I, probably contains a classical double radio source. Attention is given to the integral luminosity function for the cluster, as well as the distribution of V-R colors for its stellar objects.

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