The Coma supercluster - Analysis of Zwicky-Herzog cluster 16 in field 158

Details The Coma supercluster - Analysis of Zwicky-Herzog cluster 16 in field 158 The Coma supercluster - Analysis of Zwicky-Herzog cluster 16 in field 158

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...206...30c&link_type=abstract

Astrophysical Journal, vol. 206, May 15, 1976, pt. 1, p. 30-37.

Other

88

Cosmology, Galactic Clusters, Radial Velocity, Velocity Distribution, Luminous Intensity, Radial Distribution, Tables (Data)

Scientific paper

Radial velocities for 50 of the 52 galaxies brighter than 15.1 mag within the boundaries of Zwicky-Herzog cluster 16 in field 158 are used to establish that the region is a composite of (1) part of the Coma I cloud of the Local Supercluster, (2) part of the supercluster of which the Coma cluster is a member, (3) the NGC 4169 group, and (4) other galaxies. The Coma supercluster is detected to a radial distance from the center of the Coma cluster of 14.2 deg (31.5 Mpc for H = 55 km/s per Mpc).

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