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  Explaining temporal variations in the jet PA of the blazar OJ 287 using its BBH central engine model

Dey, L., Valtonen, M. J., Gopakumar, A., Lico, R., Gómez, J. L., Susobhanan, A., et al. (2021). Explaining temporal variations in the jet PA of the blazar OJ 287 using its BBH central engine model. \mnras, 503(3), 4400-4412. doi:10.1093/mnras/stab730.

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 Creators:
Dey, Lankeswar, Author
Valtonen, Mauri J., Author
Gopakumar, A., Author
Lico, Rocco, Author
Gómez, José L., Author
Susobhanan, Abhimanyu, Author
Komossa, S.1, Author
Pihajoki, Pauli, Author
Affiliations:
1Max Planck Institute for Radio Astronomy, Max Planck Society, ou_2205652              

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Free keywords: accretion, accretion discs, BL Lacertae objects: individual: OJ 287, galaxies: jets, black hole physics, Astrophysics - High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology
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 Dates: 2021-05
 Publication Status: Issued
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 Identifiers: DOI: 10.1093/mnras/stab730
BibTex Citekey: 2021MNRAS.503.4400D
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Title: \mnras
Source Genre: Journal
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Pages: - Volume / Issue: 503 (3) Sequence Number: - Start / End Page: 4400 - 4412 Identifier: -