Faint Structures in Low Density Regions of the Nearby Universe release_spjlicbttrh6fkcyqyr4ide4re

by U. Lindner, K.J. Fricke, J. Einasto, M. Einasto

Published in Symposium - International astronomical union by Cambridge University Press (CUP).

1999   Volume 183, p256

Abstract

We present an investigation of the galaxy distribution in the huge underdense region between the Hercules, Coma and Local Superclusters, the so-called Northern Local Void (NLV), using void statistics (for details refer to Lindner et al. this Volume). Reshift data for galaxies and poor clusters of galaxies are available in low and high density regions as well. Samples of galaxies with different morphological type and various luminosity limits have been studied separately and void catalogues have been compiled from three different luminosity limited galaxy samples for the first time. Voids have been found using the empty sphere method which has the potential to detect and describe subtle structures in the galaxy distribution. Our approach is complementary to most other methods usually used in Large–Scale Structure studies.
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