Average Spectral Energy Distributions of Blazars from Radio to Gamma-Rays

Simple item page
dc.creatorFossati, G.
dc.creatorCelotti, A.
dc.creatorGhisellini, G.
dc.creatorMaraschi, L.
dc.date1997-06-18
dc.date.accessioned2026-07-07T02:23:38Z
dc.date.available2026-07-07T02:23:38Z
dc.descriptionThe average Spectral Energy Distributions (SED) of different classes of blazars from the radio to the gamma-ray band are studied adopting a "complete-sample" approach. The SED are globally similar, despite systematic differences in specific frequency ranges, showing two broad peaks. However, i) the first and second peak occur in different frequency ranges for different objects, with a tendency for the most luminous sources to peak at lower frequencies, ii) the ratio between the two peak frequencies *seems to be constant*, iii) the luminosity ratio between the high and low frequency component increases with the bolometric luminosity.
dc.description4 pages, TeX, uses lecproc.cmm and psfig.tex, 1 figure (included), To appear in Proceedings of workshop "Relativistic jets in AGNs", Cracow, 27-30 May 1997 Also available at this URL http://www.sissa.it/~fossati/pub_list.html
dc.identifierhttps://arxiv.org/abs/astro-ph/9706190
dc.identifierhttp://arxiv.org/abs/astro-ph/9706190
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11323
dc.subjectAstrophysics
dc.titleAverage Spectral Energy Distributions of Blazars from Radio to Gamma-Rays
dc.typetext

Files

Collections

arXiv