OJ 287's December 2015 GR-model flare is linked to the emergence of jet component K, whose revised speed of 0.12 mas/yr places it at the site of the February 2017 VHE flare.
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The polarisation behaviour of OJ 287 viewed through radio, millimetre and optical observations between 2015 and 2017
OJ 287's December 2015 GR-model flare is linked to the emergence of jet component K, whose revised speed of 0.12 mas/yr places it at the site of the February 2017 VHE flare.