Radio and X-ray Emission in MOJAVE Blazars: The Case of 0106+013

Details Radio and X-ray Emission in MOJAVE Blazars: The Case of 0106+013 Radio and X-ray Emission in MOJAVE Blazars: The Case of 0106+013

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cfdd.confe.130k&link_type=abstract

Chandra's First Decade of Discovery, Proceedings of the conference held 22-25 September, 2009 in Boston, MA. Edited by Scott Wo

Physics

Agn Jets

Scientific paper

The kiloparsec-scale radio emission in the MOJAVE sample selected on the basis of relativistically boosted parsec-scale flux density, does not reveal a clear divide between quasars and BL Lac objects. The strong correlation observed between the kpc-scale lobe emission and parsec-scale apparent jet speeds highlights the crucial role played by the jet speed in determining the source radio power and thereby their Fanaroff-Riley classification, in the framework of the radio-loud unification scheme. Of the MOJAVE blazars with significant extended radio emission, nearly 80% have X-ray jets, indicative of the relevance of relativistic bulk motion in producing nonthermal X-ray emission. We present the primary findings of the kpc-scale radio study of MOJAVE blazars and discuss the preliminary results on some newly discovered X-ray jets in them, with special emphasis on the quasar 0106+013.

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