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The structure of the Hercules supercluster

Published online by Cambridge University Press:  07 February 2017

M. Tarenghi ,
W. G. Tifft ,
G. Chincarini ,
H. J. Rood  and
L. A. Thompson
M. Tarenghi
Affiliation:
LFCTR, Istituto di Fisica, Milano
W. G. Tifft
Affiliation:
Steward Observatory, University of Arizona
G. Chincarini
Affiliation:
Dept. of Physics and Astronomy, University of Oklahoma and Universita di Bologna
H. J. Rood
Affiliation:
Dept. of Astronomy, Michigan State University
L. A. Thompson
Affiliation:
Dept. of Astronomy, University of Nebraska

Extract

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Counts by Shane and Wirtanen detected a cloud of Galaxies - the Hercules Supercluster - centered at about α = 16h02m; δ = 17°00m. It is unclear whether there is a physical connection with another cloud located to the south for which no radial velocities are yet available and with the system A2197/A2199 located to the north. the latter is at slightly smaller redshift (velocities between 8000–11,000 km sec−1) than the Hercules cluster.

Type
III. Large Scale Systems
Information
Symposium - International Astronomical Union , Volume 79: The Large Scale Structure of the Universe , 1978 , pp. 263 - 265
Copyright
Copyright © Reidel 1978