Investigation of galaxies in and near the cluster A1185

Details Investigation of galaxies in and near the cluster A1185 Investigation of galaxies in and near the cluster A1185

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999arep...43...65b&link_type=abstract

Astronomy Reports, Volume 43, Issue 2, February 1999, pp.65-73

Astronomy and Astrophysics

Astronomy

Scientific paper

Results of optical, radio, and submillimeter studies of the nearby galaxy cluster A1185 are presented. Coordinates have been obtained for 115 galaxies that are either cluster members or field galaxies in the direction of A1185. Radio spectra for a number of galaxies in this cluster have been derived using observations on the RATAN-600 radio telescope at 2.7, 3.9, 7.6, 13, and 31 cm, together with data published in other studies. At the cluster center, some of the galaxies have either flat or inverted spectra. The vast majority of the galaxies display a uniform brightness distribution; i.e., they do not show any signs of structure. Sixty-four percent of the galaxies are elliptical, and 31% are spherical. The total number of blue galaxies is 22%.

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