J 2017

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

VALTONEN, Mauri, Stanislaw ZOLA, Helen JERMAK, Stefano CIPRINI, Rene HUDEC et. al.

Basic information

Original name

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

Name in Czech

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

Authors

VALTONEN, Mauri (246 Finland), Stanislaw ZOLA (616 Poland), Helen JERMAK (826 United Kingdom of Great Britain and Northern Ireland), Stefano CIPRINI (380 Italy), Rene HUDEC (203 Czech Republic), Lankeswar DEY (826 United Kingdom of Great Britain and Northern Ireland), Achamveedu GOPAKUMAR (356 India), Daniel L. REICHART (840 United States of America), Daniel B. CATON (840 United States of America), Kosmas GAZEAS (300 Greece), Katsura MATSUMOTO (392 Japan), Waldemar OGLOZA (616 Poland), Marek DRÓŻDŻ (616 Poland), Fahri ALICAVUS (792 Turkey), Oleksandr BARANSKY (804 Ukraine), Andrei BERDYUGIN (804 Ukraine), Panos BOUMIS (300 Greece), Yurii BUFAN (804 Ukraine), Bartlomiej DEBSKI (616 Poland), Huseyin ER (792 Turkey), Ahmet ERDEM (792 Turkey), Vira GODUNOVA (804 Ukraine), Shirin HAQUE (780 Trinidad and Tobago), Vivian L. HOETTE (840 United States of America), Jan JANÍK (203 Czech Republic, guarantor, belonging to the institution), Mark KIDGER (724 Spain), Tomasz KUNDERA (616 Poland), Sebastian KUROWSKI (616 Poland), Alexis LIAKOS (300 Greece), Isa MOHAMMED (780 Trinidad and Tobago), Kari NILSSON (246 Finland), Urszula PAJDOSZ (616 Poland), Vilppu PIIROLA (246 Finland), Tapio PURSIMO (724 Spain), Brandon RAJKUMAR (780 Trinidad and Tobago), Andrii O. SIMON (804 Ukraine), Michal SIWAK (616 Poland), Eda SONBAS (792 Turkey), Ian A. STEELE (826 United Kingdom of Great Britain and Northern Ireland), Volodymir V. VASYLENKO (804 Ukraine), Michal ZEJMO (616 Poland) and Pawel ZIELIŃSKI (616 Poland, belonging to the institution)

Edition

Galaxies, Switzerland, MDPI AG, 2017, 2075-4434

Other information

Language

English

Type of outcome

Článek v odborném periodiku

Field of Study

10308 Astronomy

Country of publisher

Switzerland

Confidentiality degree

není předmětem státního či obchodního tajemství

RIV identification code

RIV/00216224:14310/17:00102126

Organization unit

Faculty of Science

UT WoS

000419211800028

Keywords (in Czech)

galaxies: active; BL lacertae objects: individual (OJ 287); super massive black holes

Keywords in English

galaxies: active; BL lacertae objects: individual (OJ 287); super massive black holes

Tags

International impact, Reviewed
Změněno: 13/11/2018 10:10, RNDr. Jan Janík, Ph.D.

Abstract

V originále

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.

In Czech

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.