Abstract
Analyses for complete samples of galaxies and clusters of galaxies showed that the two-point correlation function of galaxy-galaxy and cluster- cluster have form of power law with power indices about −1.8 (Peebles, 1980; Bahcall and Soneira, 1983). Because the completeness of a sample means that we have observed completely the objects brighter than a given apparent magnitude in certain sky region. But, we know that a complete sample will be lack of faint objects at distant region. If we attempt to avoid the influences of any non-intrinsic properties on the analysis, we have to use the samples which are complete in certain interval of absolute magnitude.
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsPreview
Unable to display preview. Download preview PDF.
References
Bahcall, N. A., and Soneira, R. M. 1983, Ap. J., 270, 20.
Geller, M. J., and Huchra, J. P. 1983, Ap. J. Suppl., 52, 61.
Huchra, J. P., et al. 1982, Ap. J., 257, 423.
Peebles, P. J. E. 1980, The Large-Scale Structure of the Universe, Princeton Univ. Press.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1987 IAU
About this paper
Cite this paper
Xia, X.Y., Deng, Z.G., Zhou, Y.Y. (1987). Large-Scale Distribution of Galaxies with Different Luminosities. In: Hewitt, A., Burbidge, G., Fang, L.Z. (eds) Observational Cosmology. International Astronomical Union/ Union Astronomique Internationale, vol 124. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3853-3_35
Download citation
DOI: https://doi.org/10.1007/978-94-009-3853-3_35
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-2476-2
Online ISBN: 978-94-009-3853-3
eBook Packages: Springer Book Archive