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Effects of Distance Uncertainties on Determinations of the Galaxy Peculiar Velocity Field
Author(s) -
Nelson Padilla,
Manuel Merchán,
D. G. Lambas
Publication year - 1998
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/306114
Subject(s) - physics , galaxy , astrophysics , homogeneity (statistics) , relative velocity , peculiar velocity , radius , consistency (knowledge bases) , offset (computer science) , statistical physics , statistics , redshift , classical mechanics , mathematics , geometry , programming language , computer security , computer science
Our statistical studies comprise the mean relative velocity and velocitycorrelation for pairs of galaxies as a function of separation, and a bulk flowanalysis determined on spheres of $10 h^{-1}$ $Mpc$ radius. In order to testthe statistical analysis we use COBE normalized CDM numerical simulations withdifferent density parameters and cosmological constant and take into accountthe Tully-Fisher (TF) scatter and a possible TF zero-point offset, as well asvariations in the results of the simulations arising from different observerpositions. We compare the results of the mock catalogs with samples of spiralgalaxies taken from the Mark III catalog.Comment: 18 pages, 6 figures, to appear in Ap

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