2015
DOI: 10.3126/hj.v5i0.12814
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A Study of r- and u-Magnitude Dependence in the Spatial Orientation of Spin Vectors of SDSS Galaxies having redshift 0.10 < z < 0.11

Abstract: :We present a study of spin vector orientations of galaxies having redshift 0.10 to

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“…In the map, low redshift galaxies are found in the substructure region. High redshifted galaxies are found to be distributed randomly [16]. The color map shows that the velocity dispersion is minimum in the region where the number density of the galaxy is minimum.…”
Section: Resultsmentioning
confidence: 92%
“…In the map, low redshift galaxies are found in the substructure region. High redshifted galaxies are found to be distributed randomly [16]. The color map shows that the velocity dispersion is minimum in the region where the number density of the galaxy is minimum.…”
Section: Resultsmentioning
confidence: 92%