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Large-Scale Distribution of Galaxies with Different Luminosities

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Part of the book series: International Astronomical Union/ Union Astronomique Internationale ((IAUS,volume 124))

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.

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© 1987 IAU

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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

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  • 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

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