Galaxy clustering and the missing mass

Details Galaxy clustering and the missing mass Galaxy clustering and the missing mass

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982rspta.307..111d&link_type=abstract

(Royal Society, Discussion on the Big Bang and Element Creation, London, England, Mar. 11, 12, 1982.) Royal Society (London), Ph

Astronomy and Astrophysics

Astrophysics

2

Cosmology, Galactic Clusters, Mass Distribution, Missing Mass (Astrophysics), Red Shift, Galactic Evolution, Mass To Light Ratios, Spatial Distribution, Universe, Virgo Galactic Cluster, Virial Theorem

Scientific paper

The data on galaxy clustering is summarized, and the results of n-body simulations for understanding the large-scale structure of the Universe are briefly discussed. Evidence for the missing mass is stated, including studies of red-shift data for isolated binary galaxies, applications of the virial theorem to groups of galaxies, pair-weighted analysis of the velocity field, and the Virgo infall test. Several very strong constraints on cosmogonic scenarios are suggested, including the predominantly nonbaryonic makeup of the Universe and the importance of nongravitational, dissipative effects in separating the dark halo from the luminous galaxies.

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