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>II-Local Solution of a Spherical Homogeneous and Isotropic Universe
Radially Decelerated towards the Expansion Center: Tests on Historic Data
Sets
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II-Local Solution of a Spherical Homogeneous and Isotropic Universe
Radially Decelerated towards the Expansion Center: Tests on Historic Data
Sets
The topic of the paper is the mathematical analysis of a radially deceleratedHubble expansion from the Bahcall & Soneira void center. Such analysis, in thehypothesis of local homogeneity and isotropy, gives a particular Hubble ratiodipole structure to the expansion equation, whose solution has been studied atdifferent precision orders and successfully tested on a few historic data sets,by de Vaucouleurs (1965), by Sandage & Tammann (1975), and by Aaronson et al.(1982-86). The fittings of both the separate AA1 and AA2 samples show a goodsolution convergence as the analysis order increases, giving even coincidingsolutions when applied to 308 nearby individual galaxies (308AA1) and to 10clusters (148AA2), respectively.
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