The contribution of active galaxies to the far-infrared and submillimeter backgrounds

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dc.creatorBrusa, M.
dc.creatorComastri, A.
dc.creatorVignali, C.
dc.date2001-06-01
dc.date.accessioned2026-07-07T01:58:45Z
dc.date.available2026-07-07T01:58:45Z
dc.descriptionWe present a simple model, developed to estimate the contribution of Active Galactic Nuclei to the far--infrared background, closely linked to the AGN synthesis model for the X-ray background. According to our calculation the AGN contribution is never dominant, ranging from a few to 15 percent between 100 and 850 micron.
dc.description5 pages, 2 color figures, to appear in Proceedings of XXI Moriond Conference: "Galaxy Clusters and the High Redshift Universe Observed in X-rays", edited by D. Neumann, F.Durret, & J. Tran Thanh Van
dc.identifierhttps://arxiv.org/abs/astro-ph/0106014
dc.identifierhttp://arxiv.org/abs/astro-ph/0106014
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2843
dc.subjectAstrophysics
dc.titleThe contribution of active galaxies to the far-infrared and submillimeter backgrounds
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