Investigations of clusters of galaxies. IV - Properties of the galaxy cluster Abell 1795

Details Investigations of clusters of galaxies. IV - Properties of the galaxy cluster Abell 1795 Investigations of clusters of galaxies. IV - Properties of the galaxy cluster Abell 1795

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991an....312..149b&link_type=abstract

Astronomische Nachrichten (ISSN 0004-6337), vol. 312, no. 3, 1991, p. 149-160.

Astronomy and Astrophysics

Astronomy

4

Astronomical Photometry, Galactic Clusters, Galactic Structure, Luminous Intensity, Red Shift, Spatial Distribution

Scientific paper

The structure of the center of the galaxy cluster A 1795 and its surroundings, representing different cluster components, has been investigated in several wavelength ranges. A preferred orientation deviating about 10-20 deg from the north-south direction has been found for all cluster components. The orientation of the central cD galaxy is in good agreement with this direction, too. There seem to exist hints for antisegregation in luminosity as well as for color segregation.

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