A tentative double-jet model for blazar OJ287

We try to propose a tentative relativistic jet model for explaining the entire radio-optical phenomena observed in blazar OJ287, which has been observed quasi-periodically with a cycle of about 12yr in its optical light curve. We investigate the currently available theoretical and observational studies on the phenomena observed in OJ287 and try to find clues to its double-jet structure. It is found that the kinematic features of its superluminal components observed at 43GHz and 15GHz could be well interpreted in terms of a precessing double-jet nozzle model. And the light curves of a few optical double-peaked outbursts could be interpreted in terms of relativistic jet models. Both jets precess with the same period of 12yr, equal to the optical period and the precession of the jets could be originated from the orbital motion of the binary. Thus the masses of the binary black holes could be estimated. We also tentatively suggest a comprehensive framework for understanding the entire phenomena in OJ287 in terms of relativistic jet models.