Evolution of AGN and Stellar Formation through Radio Surveys

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dc.creatorGregorini, L.
dc.creatorPrandoni, I.
dc.date1999-10-12
dc.date.accessioned2026-07-07T02:33:47Z
dc.date.available2026-07-07T02:33:47Z
dc.descriptionThe change in the slope of the radio source counts suggests the emergence of a new population of radio galaxies at mJy and sub-mJy levels. Our understanding of such faint radio sources has advanced over the last decade through increasingly sensitive radio surveys and follow-up works at optical wavelength. The sub-mJy population seems to include both star forming galaxies and classical (AGN-powered) radio sources, but the relative importance of the two classes is still debated. Recent results are reviewed and discussed.
dc.description10 pages, 3 figures, Proceedings of XLIII Congresso Nazionale della S.A.It
dc.identifierhttps://arxiv.org/abs/astro-ph/9910201
dc.identifierhttp://arxiv.org/abs/astro-ph/9910201
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14985
dc.subjectAstrophysics
dc.titleEvolution of AGN and Stellar Formation through Radio Surveys
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