Quasar-modulated galaxy clustering in a cold dark matter universe

Details Quasar-modulated galaxy clustering in a cold dark matter universe Quasar-modulated galaxy clustering in a cold dark matter universe

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.253p..31b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 253, Dec. 1, 1991, p. 31P-34P.

Astronomy and Astrophysics

Astronomy

81

Dark Matter, Galactic Clusters, Galactic Evolution, Quasars, Astronomical Models, Red Shift, Universe

Scientific paper

The possibility that large-scale structure in the galaxy distribution is the result of quasars modulating galaxy formation in the standard CDM model is explored. Specifically, the case where radiation from high-redshift quasars is assumed to suppress galaxy formation in their neighborhood is considered. The observed quasar population can, in principle, influence large enough regions of space to reconcile the CDM model with recent measurements of large-scale structure. In such a model the observed voids should contain failed galaxies and galaxy clusters.

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