AGN and Starburst Galaxies Seen through Radio Surveys

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dc.creatorGregorini, L.
dc.creatorPrandoni, I.
dc.creatorde Ruiter, H. R.
dc.creatorParma, P.
dc.creatorVettolani, G.
dc.creatorZanichelli, A.
dc.creatorWieringa, M. H.
dc.creatorEkers, R. D.
dc.date2000-10-19
dc.date.accessioned2026-07-07T01:56:06Z
dc.date.available2026-07-07T01:56:06Z
dc.descriptionThe emergence of a new population of radio galaxies at mJy and sub-mJy levels is responsible for the change in the slope of the radio source counts. This 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. We present results from the ATESP radio survey and its optical follow-up and show that the fraction of starburst galaxies changes from ~15% at fluxes >1 mJy to >50% at lower fluxes.
dc.description6 pages and 3 ps figures. To be published in Proc. of the Conference "the New Era of Wide-Field Astronomy", held in Preston (UK), 21-24 August 2000
dc.identifierhttps://arxiv.org/abs/astro-ph/0010384
dc.identifierhttp://arxiv.org/abs/astro-ph/0010384
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1879
dc.subjectAstrophysics
dc.titleAGN and Starburst Galaxies Seen through Radio Surveys
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