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- W1491217342 abstract "A three-dimensional numerical model based on the adiabatic galaxy-formation scenario suggests that rich clusters may develop in three steps: a flat proto-supercluster (pancake) will form, long filamentary structures will originate within it, and finally large-scale flows in the filaments will give rise to clusters." @default.
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- W1491217342 date "1984-09-01" @default.
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- W1491217342 title "Rich galaxy clusters may result from large-scale motions inside superclusters" @default.
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