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Identifying the Secondary Jet in the RadioAstron Image of OJ 287

The 136 yr long optical light curve of OJ 287 is explained by a binary black hole model where the secondary is in a 12 yr orbit around the primary. Impacts of the secondary on the accretion disk of the primary generate a series of optical flares that follow a quasi-Keplerian relativistic mathematica...

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Hoofdauteurs: Mauri J. Valtonen, Lankeswar Dey, Staszek Zola, Alok C. Gupta, Shubham Kishore, Achamveedu Gopakumar, Paul J. Wiita, Minfeng Gu, Kari Nilsson, Zhongli Zhang, Rene Hudec, Katsura Matsumoto, Marek Drozdz, Waldemar Ogloza, Andrei V. Berdyugin, Daniel E. Reichart, Markus Mugrauer, Tapio Pursimo, Stefano Ciprini, Tatsuya Nakaoka, Makoto Uemura, Ryo Imazawa, Michal Zejmo, Vladimir V. Kouprianov, James W. Davidson Jr., Alberto Sadun, Jan Štrobl, Martin Jelínek, Abhimanyu Susobhanan
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: IOP Publishing 2025-01-01
Reeks:The Astrophysical Journal
Onderwerpen:
Active galactic nuclei
Online toegang:https://doi.org/10.3847/1538-4357/ae057e
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