PRIMARY BLACK HOLE SPIN IN OJ 287 AS DETERMINED BY THE GENERAL RELATIVITY CENTENARY FLARE | Zendy

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PRIMARY BLACK HOLE SPIN IN OJ 287 AS DETERMINED BY THE GENERAL RELATIVITY CENTENARY FLARE

Author(s) -

V Valtonen,

Zola,

Ciprini,

Gopakumar,

Matsumoto,

Sadakane,

Kidger,

Gazeas,

Nilsson,

Berdyugin,

Piirola,

Jermak,

Baliyan,

Alicavus,

Boyd,

M. Torrent,

Campos,

J. Carrillo Gómez,

Caton,

Chavushyan,

D'Alessio,

Debski,

Димитров,

Drozdz,

er,

Erdem,

Alex Escartin Perez,

V. Fallah Ramazani,

Filippenko,

Ganesh,

García,

Gómez Pinilla,

Gopinathan,

Haislip,

Hudec,

Hurst,

Ivarsen,

Jelínek,

Joshi,

Kagitani,

Kaur,

Keel,

LaCluyze,

Lee,

Lindfors,

Lozano De Haro,

Moore,

Mugrauer,

Naves Nogues,

Neely,

Nelson,

Ogloza,

Okano,

Pandey,

Perri,

Pihajoki,

Poyner,

Provencal,

Pursimo,

Raj Raj,

Reichart,

Reinthal,

Sadegi,

Sakanoi,

Salto González,

Sameer,

Schweyer,

Siwak,

Soldán Alfaro,

Sonbas,

Steele,

Stocke,

Strobl,

Takalo,

Tomov,

Tremosa Espasa,

Valdés,

Valero Pérez,

Verrecchia,

Webb,

Yoneda,

Zejmo,

Z. Zheng,

Telting,

Saario,

Reynolds,

Kvammen,

Gafton,

Karjalainen,

Harmanen,

Blay

Publication year - 2016

Publication title -

carolina digital repository (university of north carolina at chapel hill)

Language(s) - English

DOI - 10.17615/s1nc-y517

Subject(s) - flare , theory of relativity , primary (astronomy) , physics , astrophysics , general relativity , theoretical physics

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