J 2018

Authenticating the Presence of a Relativistic Massive Black Hole Binary in OJ 287 Using Its General Relativity Centenary Flare: Improved Orbital Parameters

DEY, L.; M.J. VALTONEN; A. GOPAKUMAR; S. ZOLA; R. HUDEC et. al.

Basic information

Original name

Authenticating the Presence of a Relativistic Massive Black Hole Binary in OJ 287 Using Its General Relativity Centenary Flare: Improved Orbital Parameters

Authors

DEY, L.; M.J. VALTONEN; A. GOPAKUMAR; S. ZOLA; R. HUDEC; P. PIHAJOKI; S. CIPRINI; K. MATSUMOTO; K. SADAKANE; M. KIDGER; K. NILSSON; S. MIKKOLA; A. SILLANPAA; L.O. TAKALO; H.J. LEHTO; A. BERDYUGIN; V. PIIROLA; H. JERMAK; K.S. BALIYAN; T. PURSIMO; D.B. CATON; F. ALICAVUS; A. BARANSKY; P. BLAY; P. BOUMIS; D. BOYD; M.C. TORRENT; F. CAMPOS; J.C. GOMEZ; S. CHANDRA; V. CHAVUSHYAN; J. DALESSIO; B. DEBSKI; M. DROZDZ (616 Poland); H. ER; A. ERDEM; A.E. PEREZ; V.F. RAMAZANI; A.V. FILIPPENKO; E. GAFTON; S. GANESH; F. GARCIA; K. GAZEAS (300 Greece); V. GODUNOVA (643 Russian Federation); F.G. PINILLA; M. GOPINATHAN; J.B. HAISLIP; J. HARMANEN; G. HURST; Jan JANÍK (203 Czech Republic, guarantor, belonging to the institution); M. JELINEK (203 Czech Republic); A. JOSHI; M. KAGITANI; R. KARJALAINEN; N. KAUR; W.C. KEEL; V.V. KOUPRIANOV; T. KUNDERA (616 Poland); S. KUROWSKI; A. KVAMMEN; A.P. LACLUYZE; B.C. LEE; A. LIAKOS; E. LINDFORS; J.L. DE HARO; M. MUGRAUER; R.N. NOGUES; A.W. NEELY; R.H. NELSON; W. OGLOZA; S. OKANO; U. PAJDOSZ-SMIERCIAK; J.C. PANDEY; M. PERRI; G. POYNER; J. PROVENCAL; A. RAJ; D.E. REICHART; R. REINTHAL; T. REYNOLDS; J. SAARIO; S. SADEGI; T. SAKANOI; J.L.S. GONZALEZ; S. SAMEER; T. SCHWEYER; A. SIMON; M. SIWAK; F.C.S. ALFARO; E. SONBAS; I. STEELE; J.T. STOCKE; J. STROBL; T. TOMOV; L.T. ESPASA; J.R. VALDES; J.V. PEREZ; F. VERRECCHIA; V. VASYLENKO; J.R. WEBB; M. YONEDA; M. ZEJMO; W. ZHENG and Pawel ZIELIŃSKI (616 Poland)

Edition

Astrophysical Journal, Chicago, University of Chicago Press, 2018, 0004-637X

Other information

Language

English

Type of outcome

Article in a journal

Field of Study

10308 Astronomy

Country of publisher

United States of America

Confidentiality degree

is not subject to a state or trade secret

References:

Impact factor

Impact factor: 5.580

RIV identification code

RIV/00216224:14310/18:00104112

Organization unit

Faculty of Science

UT WoS

000446752400011

EID Scopus

2-s2.0-85055252909

Keywords in English

black hole physics; gravitation; quasars: general; quasars: individual (OJ 287)

Tags

International impact, Reviewed
Changed: 23/4/2024 12:35, Mgr. Michal Petr

Abstract

In the original language

Results from regular monitoring of relativistic compact binaries like PSR 1913+16 are consistent with the dominant (quadrupole) order emission of gravitational waves (GWs). We show that observations associated with the binary black hole (BBH) central engine of blazar OJ 287 demand the inclusion of gravitational radiation reaction effects beyond the quadrupolar order. It turns out that even the effects of certain hereditary contributions to GW emission are required to predict impact flare timings of OJ 287. We develop an approach that incorporates this effect into the BBH model for OJ 287. This allows us to demonstrate an excellent agreement between the observed impact flare timings and those predicted from ten orbital cycles of the BBH central engine model. The deduced rate of orbital period decay is nine orders of magnitude higher than the observed rate in PSR 1913+16, demonstrating again the relativistic nature of OJ 287's central engine. Finally, we argue that precise timing of the predicted 2019 impact flare should allow a test of the celebrated black hole "no-hair theorem" at the 10% level.