Strong compact and extended radio sources at high redshifts

Details Strong compact and extended radio sources at high redshifts Strong compact and extended radio sources at high redshifts

Apr 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..470..270r&link_type=abstract

The 9th astrophysics conference: After the dark ages, when galaxies were young (the Universe at 2<Z<5). AIP Conference Proceedi

Astronomy and Astrophysics

Astrophysics

Radio Sources, Observational Cosmology

Scientific paper

Previously we have discussed models for strong compact and extended radio sources. In this paper we describe how the nature of these models is expected to depend on redshift and make a preliminary attempt to connect theory with observations. In particular we predict that the number of strong compact radio sources should decline more rapidly with redshift than the number of quasars. We also give physical explanations for the steepening of the average spectral index of radio sources with redshift as well as their smaller dimensions.

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