The evolution of radio galaxy emission line regions: Breaking the P-z degeneracy

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dc.creatorInskip, K. J.
dc.creatorBest, P. N.
dc.creatorLongair, M. S.
dc.date2002-08-29
dc.date.accessioned2026-07-07T02:04:51Z
dc.date.available2026-07-07T02:04:51Z
dc.descriptionThe ionization and kinematic properties of the emission line regions of three subsamples of 6C and 3CR radio galaxies have been compared. The degeneracy between redshift and radio power is broken, and the relative importance of radio power (P), radio size (D) and redshift (z) for the emission line region properties is determined.
dc.description2 pages, 1 figure, to be published in "A New Era in Cosmology" ASP conf. ser. Eds. T. Shanks and N. Metcalfe
dc.identifierhttps://arxiv.org/abs/astro-ph/0208550
dc.identifierhttp://arxiv.org/abs/astro-ph/0208550
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4922
dc.subjectAstrophysics
dc.titleThe evolution of radio galaxy emission line regions: Breaking the P-z degeneracy
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