A deficiency of large-scale pairs among nearby quasars

Details A deficiency of large-scale pairs among nearby quasars A deficiency of large-scale pairs among nearby quasars

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...387l..13r&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 387, March 1, 1992, p. L13-L15.

Other

Galactic Clusters, Galactic Evolution, Interacting Galaxies, Quasars, Hubble Constant, Red Shift

Scientific paper

The two-point correlation function for quasars within a redshift of 0.19 shows a significant deficit of pairs at a comoving coordinate separation of 0.17, when evaluated in the Einstein-de Sitter model universe. This separation, if referred to the present epoch, corresponds to a physical scale of 510/h Mpc, if the Hubble constant H(0) = 100h km/s Mpc. No other significant departures from zero are found out to a comoving separation of 0.24.

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