Young radio-loud AGN: A new sample at low redshift

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dc.creatorSnellen, I. A. G.
dc.creatorMack, K. -H.
dc.creatorTschager, W.
dc.creatorSchilizzi, R. T.
dc.date2000-09-29
dc.date.accessioned2026-07-07T01:55:42Z
dc.date.available2026-07-07T01:55:42Z
dc.descriptionWe report on the investigation of a complete sample of young radio-loud AGN at z<0.25, selected using the new comprehensive radio surveys and the optical APM/POSS-I catalog. This new sample will provide a unique opportunity for statistical studies of the early evolution of radio-loud AGN, free of cosmological evolution effects. In particular, their local luminosity function, linear-size and dynamical age distributions, may strongly constrain possible evolution scenarios. In addition, this new sample is well suited for statistical studies of other important properties, like their X-ray and infrared emissions, optical cluster environments, and neutral hydrogen in absorption towards the compact radio sources.
dc.descriptionLaTeX, 4 pages, 2 figs: To appear in the Proceedings of the 5th EVN Symposium. Eds. J. Conway, A. Polatidis, R.Booth., Onsala Space Observatory, Chalmers Technical University, Gothenburg, Sweden (2000)
dc.identifierhttps://arxiv.org/abs/astro-ph/0009484
dc.identifierhttp://arxiv.org/abs/astro-ph/0009484
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1749
dc.subjectAstrophysics
dc.titleYoung radio-loud AGN: A new sample at low redshift
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