Polarization and Spectral Energy Distribution in OJ 287 during the 2016/17 Outbursts
Mauri Valtonen; Stanislaw Zola; Helen Jermak; Stefano Ciprini; Rene Hudec; Lankeswar Dey; Achamveedu Gopakumar; Daniel L. Reichart; Daniel B. Caton; Kosmas Gazeas; Katsura Matsumoto; Waldemar Ogloza; Marek Drozdz; Fahri Alicavus; Oleksandr Baransky; Andrei Berdyugin; Panos Boumis; Yurii Bufan; Bartlomiej Debski; Huseyin Er; Ahmet Erdem; Vira Godunova; Shirin Haque; Vivian L. Hoette; Jan Janik; Mark Kidger; Tomasz Kundera; Sebastian Kurowski; Alexis Liakos; Isa Mohammed; Kari Nilsson; Urszula Pajdosz; Vilppu Piirola; Tapio Pursimo; Brandon Rajkumar; Andrii O. Simon; Michal Siwak; Eda Sonbas; Ian A. Steele; Volodymir V. Vasylenko; Michal Zejmo; Pawel Zielinski
Polarization and Spectral Energy Distribution in OJ 287 during the 2016/17 Outbursts
MDPI AG
Julkaisun pysyvä osoite on:
https://urn.fi/URN:NBN:fi-fe2021042718387
https://urn.fi/URN:NBN:fi-fe2021042718387
Tiivistelmä
We report optical photometric and polarimetric observations of the
blazar OJ 287 gathered during 2016/17. The high level of activity,
noticed after the General Relativity Centenary flare, is argued to be
part of the follow-up flares that exhibited high levels of polarization
and originated in the primary black hole jet. We propose that the
follow-up flares were induced as a result of accretion disk
perturbations, traveling from the site of impact towards the primary
SMBH. The timings inferred from our observations allowed us to estimate
the propagation speed of these perturbations. Additionally, we make
predictions for the future brightness of OJ 287.
Kokoelmat
- Rinnakkaistallenteet [27094]