Radio galaxies and structure formation

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dc.creatorPeacock, J. A.
dc.date1997-12-04
dc.date.accessioned2026-07-07T02:25:29Z
dc.date.available2026-07-07T02:25:29Z
dc.descriptionThis review discusses three ways in which radio galaxies and other high-redshift objects can give us information on the nature and statistics of cosmological inhomogeneities, and how they have evolved between high redshift and the present: (1) The present-day spatial distribution and clustering of radio galaxies; (2) The evolution of radio-galaxy clustering and biased clustering at high redshift; (3) Measuring density perturbation spectra from the abundances of high-redshift galaxies.
dc.descriptionReview at the KNAW colloquium `The most distant radio galaxies', Amsterdam, October 1997. Reidel in press
dc.identifierhttps://arxiv.org/abs/astro-ph/9712068
dc.identifierhttp://arxiv.org/abs/astro-ph/9712068
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11894
dc.subjectAstrophysics
dc.titleRadio galaxies and structure formation
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