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Millimetre Continuum Variations, VLBI Structure and Gamma-rays: Investigating Shocked Jet Physics

Published online by Cambridge University Press:  05 March 2013

E. Valtaoja*
Affiliation:
Tuorla Observatory, FIN-21500 Piikkiö, Finland Department of Physics, Turku University, FIN-20100 Turku, Finland
T. Savolainen
Affiliation:
Tuorla Observatory, FIN-21500 Piikkiö, Finland
K. Wiik
Affiliation:
Tuorla Observatory, FIN-21500 Piikkiö, Finland Metsähovi Radio Observatory, Helsinki University of Technology, FIN-02540 Kylmälä, Finland
A. Lähteenmäki
Affiliation:
Metsähovi Radio Observatory, Helsinki University of Technology, FIN-02540 Kylmälä, Finland
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Abstract

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We compare the total flux density variations and the VLBI structural variations in a sample of 27 gamma-ray blazars. We find that all the radio variations are due to shocks; the flux of the underlying jet remains constant. A large fraction of the shocks grow and fade within the innermost 0.1 mas, appearing only as ‘core flares’. Comparisons with the EGRET data show that gamma-ray flares must come from the shocks, not from the jet. At the time of an EGRET flare, the shock is typically already over a parsec downstream from the radio core, beyond the accretion disk and/or the broad line region (BLR) photon fields. Thus, present models for gamma-ray production are inadequate, since they typically model the gamma-ray inverse Compton flux as coming from the jet, with significant disk or BLR external Compton components.

Type
Research Article
Copyright
Copyright © Astronomical Society of Australia 2002

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