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The 2015 outburst of the OJ287 blazar




AuthorsValtonen, M., Zola, S., Gopakumar, A., Gazeas, K., Ogloza, W., Drozdz, M., Siwak, M., Debski, B., Dalessio, J., Sadakane, K., Kidger, M., Nilsson, K., Berdyugin, A., Lindfors, E., Takalo, L., Baliyan, K., Mugrauer, M., Alicavus, F., Erdem, A., Provencal, J., Webb, J., Zejmo, M., Sonbas, E., Er, H., Keel, W., Schweyer, T.

Publication year2015

Volume8378

First page 1

Last page1

Web address http://www.astronomerstelegram.org/?read=8378(external)


Abstract

A model that contains a massive BH binary was proposed to explain the double peaked quasi-periodical (roughly about 12 years) outbursts of the blazar OJ287.




Last updated on 2024-26-11 at 17:17