Polarization and Spectral Energy Distribution in OJ 287 during the 2016/17 Outbursts

Valtonen, Mauri; Zola, Stanislaw; Jermak, Helen; Ciprini, Stefano; Hudec, Rene; Dey, Lankeswar; Gopakumar, Achamveedu; Reichart, Daniel; Caton, Daniel; Gazeas, Kosmas; Matsumoto, Katsura; Ogloza, Waldemar; Drozdz, Marek; Alicavus, Fahri; Baransky, Oleksandr; Berdyugin, Andrei; Boumis, Panos; Bufan, Yurii; Debski, Bartlomiej; Er, Hüseyin; Erdem, Ahmet; Godunova, Vira; Haque, Shirin; Hoette, Vivian; Janik, Jan; Kidger, Mark; Kundera, Tomasz; Kurowski, Sebastian; Liakos, Alexis; Mohammed, Isa; Nilsson, Kari; Pajdosz, Urszula; Piirola, Vilppu; Pursimo, Tapio; Rajkumar, Brandon; Simon, Andrii; Siwak, Michal; Sonbas, Eda; Steele, Ian; Vasylenko, Volodymir; Zejmo, Michal; Zielinski, Pawel

doi:10.3390/galaxies5040083

Polarization and Spectral Energy Distribution in OJ 287 during the 2016/17 Outbursts

Atıf İçin Kopyala

Valtonen M., Zola S., Jermak H., Ciprini S., Hudec R., Dey L., ...Daha Fazla

GALAXIES, cilt.5, 2017 (ESCI)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 5
Basım Tarihi: 2017
Doi Numarası: 10.3390/galaxies5040083
Dergi Adı: GALAXIES
Derginin Tarandığı İndeksler: Emerging Sources Citation Index (ESCI), Scopus
Anahtar Kelimeler: galaxies: active, BL lacertae objects: individual (OJ 287), super massive black holes, BLACK-HOLE, OJ-287
Atatürk Üniversitesi Adresli: Evet

Özet

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.