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Title:
Radio spectra of intermediate-luminosity broad-line radio galaxies .
Authors:
Angelakis, E.; Kadler, M.; Lewis, K.; Sambruna, R. M.; Eracleous, M.; Zensus, J. A.
Affiliation:
AA( Max-Plank-Institut für Radioastronomie, Auf dem Hügel 69, DE-53121 Bonn, Germany ), AB(Dr. Karl Remeis-Observatory,University of Erlangen-Nuremberg, Sternwartstrasse 7, Bamberg, 96049, Germany; CRESST/NASA Goddard Space Flight Center, 662 Greenbelt, MD 20721, USA; Universities Space Research Association, 10211 Wincopin Circle, Suite 500 Columbia, MD 21044, USA), AC(Department of Physics & Astronomy, Dickinson College, Carlisle, PA 17013, USA), AD(Astroparticle Physics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA), AE(Department of Astronomy & Astrophysics, The Pennsylvania State University, University Park, PA 16802, USA), AF( Max-Plank-Institut für Radioastronomie, Auf dem Hügel 69, DE-53121 Bonn, Germany )
Publication:
Memorie della Societa Astronomica Italiana, v.79, p.1038 (2008)
Publication Date:
00/2008
Origin:
MmSAI
Keywords:
Galaxies: active, Galaxies: nuclei, Radio continuum: galaxies
Bibliographic Code:
2008MmSAI..79.1038A

Abstract

Within 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.

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