Počet záznamů: 1
Observational Implications of OJ 287's Predicted 2022 Disk Impact in the Black Hole Binary Model
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SYSNO ASEP 0575399 Druh ASEP J - Článek v odborném periodiku Zařazení RIV J - Článek v odborném periodiku Poddruh J Článek ve WOS Název Observational Implications of OJ 287's Predicted 2022 Disk Impact in the Black Hole Binary Model Tvůrce(i) Valtonen, M.J. (FI)
Dey, L. (IN)
Gopakumar, A. (IN)
Hudec, René (ASU-R) RID, ORCID
Jelínek, Martin (ASU-R) ORCID
Štrobl, Jan (ASU-R) ORCID, RIDCelkový počet autorů 28 Číslo článku 82 Zdroj.dok. Galaxies. - : MDPI
Roč. 11, č. 4 (2023)Poč.str. 22 s. Forma vydání Online - E Jazyk dok. eng - angličtina Země vyd. CH - Švýcarsko Klíč. slova BL Lacertae objects ; supermassive black holes ; accretion discs Obor OECD Astronomy (including astrophysics,space science) Způsob publikování Open access Institucionální podpora ASU-R - RVO:67985815 UT WOS 001055641700001 EID SCOPUS 85169118890 DOI 10.3390/galaxies11040082 Anotace 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. Pracoviště Astronomický ústav Kontakt Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Rok sběru 2024 Elektronická adresa https://hdl.handle.net/11104/0345985
Počet záznamů: 1