Radio spectra of intermediate-luminosity broad-line radio galaxies

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dc.creatorAngelakis, E.
dc.creatorKadler, M.
dc.creatorLewis, K.
dc.creatorSambruna, R. M.
dc.creatorEracleous, M.
dc.creatorZensus, J. A.
dc.date2008-07-25
dc.date.accessioned2026-07-07T09:52:56Z
dc.date.available2026-07-07T09:52:56Z
dc.descriptionWithin the context of investigating possible differences between the mechanisms at play in Radio Loud AGN and those in Radio Quiet ones, we study the spectral characteristics of a selected sample of Intermediate-Luminosity Broad-Line Radio Galaxies in X-rays, optical, IR and radio. Here, we present the radio spectra acquired with the 100-m radio telescope in Effelsberg between 2.6 and 32 GHz. These measurements reveal a large variety of spectral shapes urging for radio imaging that would disclose the source morphology. Such studies could potentially discriminate between different mechanisms.
dc.description4 pages, 1 figure, to appear in the proceedings of the Conference "The Central Kiloparsec: Active Galactic Nuclei and Their Hosts", Ierapetra 4-6 June 2008, Greece, Memorie della Societa Astronomica Italiana
dc.identifierhttps://arxiv.org/abs/0807.4102
dc.identifierhttp://arxiv.org/abs/0807.4102
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/165775
dc.subjectAstrophysics
dc.titleRadio spectra of intermediate-luminosity broad-line radio galaxies
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