Galaxies (Nov 2017)

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

DOI
https://doi.org/10.3390/galaxies5040083
Journal volume & issue
Vol. 5, no. 4
p. 83

Abstract

Read online

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, travelling 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.

Keywords