paper

Rotation of the optical polarization angle associated with the 2008 γ-ray flare of blazar w comae

arXiv:1408.1339 · doi:10.1088/0004-637X/794/1/54

Abstract

An --band photopolarimetric variability analysis of the TeV bright blazar W Comae, between 2008 February 28 and 2013 May 17, is presented. The source showed a gradual tendency to decrease its mean flux level with a total change of ~3~mJy. A maximum and minimum brightness states in the -band of 14.250.04 and 16.520.1~mag respectively were observed, corresponding to a maximum variation of F = 5.40 mJy. We estimated a minimum variability timescale of t=3.3 days. A maximum polarization degree =33.8\%1.6\%, with a maximum variation of P = 33.2\%, was found. One of our main results is the detection of a large rotation of the polarization angle from 78\degr to 315\degr (237\degr) that coincides in time with the -ray flare observed in 2008 June. This result indicates that both optical and -ray emission regions could be co-spatial. During this flare, a correlation between the -band flux and polarization degree was found with a correlation coefficient of 0.11. From the Stokes parameters we infer the existence of two optically thin synchrotron components that contribute to the polarized flux. One of them is stable with a constant polarization degree of 11\%. Assuming a shock-in jet model during the 2008 flare, we estimated a maximum Doppler factor and a minimum of ; a minimum viewing angle of the jet 2\degr.0; and a magnetic field 0.12~G.

Accepted in ApJ,34 pages,6 figures,4 tables. arXiv admin note: text overlap with arXiv:1304.2819

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Rotation of the optical polarization angle associated with the 2008 γ-ray flare of blazar w comae · wovepaper