Observational Implications of OJ 287's Predicted 2022 Disk Impact in the Black Hole Binary Model
Abstract
We present a summary of the results of the OJ 287 observational campaign, which was carried out during the 2021/2022 observational season. This season is special in the binary model because the major axis of the precessing binary happens to lie almost exactly in the plane of the accretion disc of the primary. This leads to pairs of almost identical impacts between the secondary black hole and the accretion disk in 2005 and 2022. In 2005, a special flare called "blue flash" was observed 35 days after the disk impact, which should have also been verifiable in 2022. We did observe a similar flash and were able to obtain more details of its properties. We describe this in the framework of expanding cloud models. In addition, we were able to identify the flare arising exactly at the time of the disc crossing from its photo-polarimetric and gamma-ray properties. This is an important identification, as it directly confirms the orbit model. Moreover, we saw a huge flare that lasted only one day. We may understand this as the lighting up of the jet of the secondary black hole when its Roche lobe is suddenly flooded by the gas from the primary disk. Therefore, this may be the first time we directly observed the secondary black hole in the OJ 287 binary system.
Keywords
Cite
@article{arxiv.2308.01878,
title = {Observational Implications of OJ 287's Predicted 2022 Disk Impact in the Black Hole Binary Model},
author = {Mauri J. Valtonen and Lankeswar Dey and Achamveedu Gopakumar and Staszek Zola and Anne Lähteenmäki and Merja Tornikoski and Alok C. Gupta and Tapio Pursimo and Emil Knudstrup and Jose L. Gomez and Rene Hudec and Martin Jelínek and Jan Štrobl and Andrei V. Berdyugin and Stefano Ciprini and Daniel E. Reichart and Vladimir V. Kouprianov and Katsura Matsumoto and Marek Drozdz and Markus Mugrauer and Alberto Sadun and Michal Zejmo and Aimo Sillanpää and Harry J. Lehto and Kari Nilsson and Ryo Imazawa and Makoto Uemura},
journal= {arXiv preprint arXiv:2308.01878},
year = {2023}
}
Comments
24 pages, 13 figures, published in Galaxies as part of the Special Issue Distant Glowing Objects: Quest for Quasars