Galaxy correlations at high redshift and the environment of quasars

Details Galaxy correlations at high redshift and the environment of quasars Galaxy correlations at high redshift and the environment of quasars

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.223..173p&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 223, Nov. 1, 1986, p. 173-176.

Mathematics

Probability

6

Absorption Spectra, Correlation, Galactic Clusters, Quasars, Red Shift, Probability Theory

Scientific paper

In close line-of-sight pairs of quasars absorption lines may be seen in the spectrum of the further quasar at a redshift corresponding to that of the nearer quasar. This is indicative of the presence of an intervening galaxy belonging to the same cluster as the (galaxy containing the) nearer quasar. The likelihood of this occurring is calculated in terms of the galaxy correlation function and it is found that present results already suggest that quasars at redshifts above one must be associated with rich clusters.

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