Multiwavelength Observations of 6 FSRQ in 2008-2012

I. S. Troitskiy, D. A. Morozova, S. G. Jorstad, V. M. Larionov, A. P. Marscher, I. Agudo, D. A. Blinov, P. S. Smith

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

We present results of 4 years of VLBA monitoring along with γ-ray and optical R-band photometric observations of 6 blazars (0420-014, 1156+295, 1222+216, PKS 1510-089, 1633+382 and CTA 102). We have analyzed total intensity images obtained with the VLBA at 43 GHz and investigated kinematic evolution of the pc-scale jets of the sources. For all sources we compare flux variations in the VLBI core and bright superluminal knots with γ-ray and optical light curves. The majority of γ-ray flares are coincident with the appearance of a new superluminal knot and/or a flare in the millimeter-wave core and at optical wavelengths. These results support the conclusion that for many flares in blazars the region of the enhanced γ-ray and optical emission is located in the vicinity or downstream of the mm-wave VLBI core.

Original languageEnglish (US)
Title of host publicationMultiwavelength AGN Surveys and Studies
PublisherCambridge University Press
Pages249-251
Number of pages3
EditionS304
ISBN (Print)9781107045248
DOIs
StatePublished - Jul 2014
Externally publishedYes

Publication series

NameProceedings of the International Astronomical Union
NumberS304
Volume9
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

Keywords

  • multiwavelength observations
  • pc-scale jet kinematics
  • γ-bright blazars

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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