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- W1988791317 abstract "The observed distribution of light in the Local Supercluster has been used to determine the expected velocities of galaxies if the assumptions are valid that nonexpansion motions are generated by gravitational perturbations and that mass is distributed like the light. Since detailed knowledge of the light distribution extends to only 3000 km s −1 , three extra sources are added at large distances: one associated with the Great Attractor, one loosely with the Perseus-Pisces Supercluster region, and one with the Shapley Concentration at a distance corresponding to 13,800 km s −1" @default.
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- W1988791317 date "1992-05-01" @default.
- W1988791317 modified "2023-10-16" @default.
- W1988791317 title "Nearby galaxy flows modeled by the light distribution" @default.
- W1988791317 doi "https://doi.org/10.1086/171322" @default.
- W1988791317 hasPublicationYear "1992" @default.
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