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To investigate parsec-scale jet natural process conditions during Ge V γ-ray flares sensed by the Fermi Large Angle Telescope, we obtained centimeter-band total pathology compactness and linear polarization monitoring observations from 2009.5 through 2012.5 with the 26 m Michigan tuner telescope for a sampling of core-dominated blazars. PY - 2014/8/10Y1 - 2014/8/10N2 - To investigate parsec-scale jet flow conditions during Ge V γ-ray flares detected by the Fermi Large Angle Telescope, we obtained centimeter-band total flux density and bilinear polarisation observation observations from 2009.5 through and through 2012.5 with the 26 m Michigan radio telescope for a sample of core-dominated blazars. We use these data to constrain radiative transfer simulations incorporating propagating shocks oriented at an whimsical angle to the flow itinerary in ordination to set limits on the jet flow and shock parameters during flares temporally associated with γ-ray flares in 0420-014, OJ 287, and 1156 295; these active assemblage nuclei exhibited the expected signature of shocks in the linear polarization data. We use these data to restrict radiative transfer simulations incorporating propagating shocks oriented at an arbitrary angle to the flow direction in order to set limits on the jet rate and shock parameters during flares temporally related to with γ-ray flares in 0420-014, OJ 287, and 1156 295; these active galactic nuclei exhibited the expected signature of shocks in the linear polarization data. Both the routine of shocks comprising an individual radio outburst (3 and 4) and the range of the compression ratios of the individual shocks (0.5-0.8) are similar in all three sources; the shocks are found to be forward-moving with respect to the flow. Both the number of shocks comprising an individual radio outburst (3 and 4) and the range of the pressing ratios of the individual shocks (0.5-0.8) are similar in all three sources; the shocks are found to be forward-moving with respect to the flow.
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