G. F. Paraschos

The connection between $\gamma$-ray flares and blazars is a topic of active research, with few sources exhibiting distinct enough such outbursts to be able to conclusively connect them to features in their jet morphology. Here we present an investigation of the sole $\gamma$-ray flare of the blazar OJ 248 thus far, in association with its jet structure, as revealed by very long baseline interferometry (VLBI). We find that throughout the course of the $\gamma$-ray flare, the fractional linear polarisation increases in the jet of OJ 248, and the VLBI electric vector position angles (EVPAs) turn perpendicular to the bulk jet flow. We interpret this behaviour as a moving shock, travelling through a recollimation shock and upscattering photons via the inverse Compton scattering process, producing a $\gamma$-ray flare; we discuss possible mechanisms. Our hypothesised shock-shock interaction scenario is a viable mechanism to induce such EVPA rotations in both optical and radio bands.