Modelling the radio to X-ray SED of galaxies

Simple item page
dc.creatorSilva, Laura
dc.creatorBressan, Alessandro
dc.creatorGranato, Gian Luigi
dc.creatorPanuzzo, Pasquale
dc.date2001-06-07
dc.date.accessioned2026-07-07T01:58:51Z
dc.date.available2026-07-07T01:58:51Z
dc.descriptionWe present our model to interpret the SED of galaxies. The model for the UV to sub-mm SED is already well established (Silva et al 1998). We remind here its main features and show some applications. Recently we have extended the model to the radio range (Bressan et al 2001), and we have started to include the X-ray emission from the stellar component.
dc.description4 pages, to be published in "The link between stars and cosmology", 26-30 March, 2001, Puerto Vallarta, Mexico, by Kluwer, eds. M. Chavez, A. Bressan, A. Buzzoni, and D. Mayya
dc.identifierhttps://arxiv.org/abs/astro-ph/0106128
dc.identifierhttp://arxiv.org/abs/astro-ph/0106128
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2878
dc.subjectAstrophysics
dc.titleModelling the radio to X-ray SED of galaxies
dc.typetext

Files

Collections

arXiv