Abstract
The redshifts of more than 600 clusters of galaxies have been compiled from the literature in order to study the large-scale distribution of these objects. Because this sample is more complete to larger distances than that of individual galaxies the volume investigated for distribution of extragalactic objects is extended relative to previous papers. For high galactic latitudes the sample is nearly complete for z ≤ 0.06 and the completeness is sufficient in order to recognize the design up to about z=0.12. In the figure example of the distribution of clusters is shouwn (•: ABELL clusters of richness class R ≥ 1; •: ABELL clusters of richness class R = O and non-ABELL clusters).
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
BAHCALL, N.A., and SONEIRA, R.M.: 1982, Astrophys. J. 262, 419.
DAVIS, M., HUCHRA, J., LATHAM, D.W., and TONRY, J.: 1982, Astrophys. J. 253, 423.
KIRSHNER, R.P., OEMLER, A.J., SCHECHTER, P.L., and SHECTMAN, S.A.: 1981, Astrophys. J. 248, L57.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1984 D. Reidel Publishing Company
About this chapter
Cite this chapter
Schmidt, KH. (1984). On the Large-Scale Distribution of Clusters of Galaxies. In: Mardirossian, F., Giuricin, G., Mezzetti, M. (eds) Clusters and Groups of Galaxies. Astrophysics and Space Science Library, vol 111. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-6412-9_14
Download citation
DOI: https://doi.org/10.1007/978-94-009-6412-9_14
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-009-6414-3
Online ISBN: 978-94-009-6412-9
eBook Packages: Springer Book Archive