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Typical Scales in Distribution of IRAS Galaxies
Published online by Cambridge University Press: 25 May 2016
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Typical scales in the distribution of IRAS galaxies have been searched for with the unnormalized pair count method given by Mo et al.1. Samples consist of a) galaxies from QDOT with | b | ≥ 20°; b) galaxies from the IRAS faint source catalog(FSC) with f60 ≥ 0.3 Jy and | b | ≥ 30°. Galaxies with b ≥ 0 and b ≤ 0 were treated as independent samples in our analysis.
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- IV. Structure Formation and Dark Matter
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- Copyright © Kluwer 1999