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The Horologium Supercluster

Published online by Cambridge University Press:  04 August 2017

G. Chincarini ,
M. Tarenghi ,
H. Sol ,
P. Crane ,
J. Manousoyannaki  and
J. Materne
G. Chincarini
Affiliation:
University of Oklahoma European Southern Observatory
M. Tarenghi
Affiliation:
European Southern Observatory
H. Sol
Affiliation:
European Southern Observatory
P. Crane
Affiliation:
European Southern Observatory
J. Manousoyannaki
Affiliation:
University of Oklahoma
J. Materne
Affiliation:
Technische Universität, Berlin

Extract

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We measured redshifts for a random subsample of 286 objects, m (Shapley) ≤ 16.5, drawn from the catalogue of the Horologium region published by Shapley. The distribution of the sample objects on the celestial sphere is shown in Fig. 1, the characteristics of the redshift distribution are represented in Figs. 2 and 3.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 104: Early Evolution of the Universe and Its Present Structure , 1983 , pp. 297 - 298
Copyright
Copyright © Reidel 1983 

References

Chincarini, G., 1982. Summer School of Cosmology and Relativity. Rio de Janeiro, January 1982, preprint.Google Scholar
Chincarini, G., Giovanelli, R. and Haynes, M., 1982, submitted to A.A. Google Scholar
Shapley, H., 1935, Annals of Harvard College Observations, Vol. 88, No. 5.Google Scholar