Authenticating the Presence of a Relativistic Massive Black Hole Binary in OJ 287 Using Its General Relativity Centenary Flare: Improved Orbital Parameters-Reference-Cited by-同舟云学术

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

Published:2018-10-05 Issue:1 Volume:866 Page:11
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Dey Lankeswar^ORCID,Valtonen M. J.^ORCID,Gopakumar A.,Zola S.,Hudec R.,Pihajoki P.,Ciprini S.,Matsumoto K.,Sadakane K.,Kidger M.,Nilsson K.^ORCID,Mikkola S.,Sillanpää A.,Takalo L. O.,Lehto H. J.,Berdyugin A.,Piirola V.,Jermak H.,Baliyan K. S.^ORCID,Pursimo T.,Caton D. B.,Alicavus F.,Baransky A.,Blay P.,Boumis P.,Boyd D.,Torrent M. Campas,Campos F.,Gómez J. Carrillo,Chandra S.^ORCID,Chavushyan V.^ORCID,Dalessio J.,Debski B.,Drozdz M.,Er H.,Erdem A.,Pérez A. Escartin,Ramazani V. Fallah,Filippenko A. V.^ORCID,Gafton E.,Ganesh S.^ORCID,Garcia F.,Gazeas K.^ORCID,Godunova V.,Pinilla F. Gómez,Gopinathan M.,Haislip J. B.,Harmanen J.,Hurst G.,Janík J.,Jelinek M.,Joshi A.,Kagitani M.,Karjalainen R.^ORCID,Kaur N.,Keel W. C.,Kouprianov V. V.,Kundera T.,Kurowski S.,Kvammen A.,LaCluyze A. P.,Lee B. C.^ORCID,Liakos A.^ORCID,Lindfors E.,de Haro J. Lozano,Mugrauer M.,Nogues R. Naves,Neely A. W.,Nelson R. H.,Ogloza W.,Okano S.,Pajdosz-Śmierciak U.,Pandey J. C.,Perri M.,Poyner G.,Provencal J.,Raj A.,Reichart D. E.,Reinthal R.,Reynolds T.,Saario J.,Sadegi S.,Sakanoi T.,González J.-L. Salto,Sameer ,Schweyer T.,Simon A.,Siwak M.,Alfaro F. C. Soldán,Sonbas E.^ORCID,Steele I.^ORCID,Stocke J. T.,Strobl J.,Tomov T.,Espasa L. Tremosa,Valdes J. R.,Pérez J. Valero,Verrecchia F.,Vasylenko V.,Webb J. R.^ORCID,Yoneda M.^ORCID,Zejmo M.,Zheng W.^ORCID,Zielinski P.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/866/i=1/a=11/pdf

Reference45 articles.

1. Gravitational two-body problem with arbitrary masses, spins, and quadrupole moments

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5. Gravitational wave tails and binary star systems

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