A comparison between the radio and the X-ray spectra of broad-line radio galaxies

E. Angelakis, M. Kadler, K. Lewis, R. M. Sambruna, M. Eracleous, J. A. Zensus

Research output: Contribution to journalConference article

1 Scopus citations

Abstract

We present the spectral characteristics of a sample of Intermediate- Luminosity Broad-Line Radio Galaxies in X- rays, optical and radio. Here, we focus on the radio spectra acquired with the 100 m radio telescope in Effelsberg between 2.6 GHz and 32 GHz. These measurements reveal different spectral shapes urging for radio imaging that would disclose the source morphology. Comparing them with the X-ray spectra acquired with XMM-Newton, we find that sources with steep radio spectrum are heavily obscured whereas flat spectrum ones appear unabsorbed in accordance with unified scheme.

Original languageEnglish (US)
Pages (from-to)522-525
Number of pages4
JournalAIP Conference Proceedings
Volume1085
DOIs
Publication statusPublished - Apr 13 2009
Event4th International Meeting on High Energy Gamma-Ray Astronomy - Heidelberg, Germany
Duration: Jul 7 2008Jul 11 2008

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All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

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