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Superclusters as nondissipative pancakes: flattening

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/160605· OSTI ID:6080201
The formation and dynamical evolution of flat superclusters (SCs) out of adiabatic perturbations of the Zel'dovich type are studied by means of N-body simulations in an Einstein--de Sitter universe, and by an approximate model in an open universe. A nondissipative formation scenario, in which galaxies or other substructures form prior to the collapse of SCs from small-scale perturbations, is found to be compatible with the observed flattening of the Local Supercluster (LSC) and of external SCs, and with their pancake-halo structure. In the best fitting model the LSC has collapsed in one dimension only recently, where 20--50% of the galaxies have crossed the plane by now, corresponding to a caustic at 0
OSTI ID:
6080201
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 264:2; ISSN ASJOA
Country of Publication:
United States
Language:
English

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