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Constraining the physical conditions in the jets of γ-ray flaring blazars using centimeter-band polarimetry and radiative transfer simulations. I. data and models for 0420-014, OJ 287, and 1156+295 — The University of Michigan


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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 one-dimensional optical phenomenon monitoring observations from 2009.5 done 2012.5 with the 26 m Michigan tuner telescope for a sample 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 enrico fermi bulky Angle Telescope, we obtained centimeter-band unit flux density and lineal polarization watching observations from 2009.5 through and through 2012.5 with the 26 m Michigan radio scope for a sample of core-dominated blazars. We use these data to cumber radiative transfer simulations incorporating propagating shocks orientating at an arbitrary angle to the flow direction in ordering 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 galactic nuclei exhibited the expected mode of shocks in the simple polarization data. We use these data to confine radiative transfer simulations incorporating propagating shocks oriented at an arbitrary angle to the movement direction in order 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 galactic nuclei exhibited the expected signature of shocks in the linear polarization data. Both the number of shocks comprising an individual radio outburst (3 and 4) and the range of the shrinkage ratios of the individualistic shocks (0.5-0.8) are similar in all three sources; the shocks are constitute to be forward-moving with regard to the flow. some the number of shocks comprising an single radio happening (3 and 4) and the reach of the compression ratios of the single shocks (0.5-0.8) are similar in all three sources; the shocks are found to be forward-moving with esteem to the flow.
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