THE STRUCTURE AND EMISSION MODEL OF THE RELATIVISTIC JET IN THE QUASAR 3C 279 INFERRED FROM RADIO TO HIGH-ENERGY γ-RAY OBSERVATIONS IN 2008-2010

M. Hayashida; C. S. Buemi; S. Ciprini; J. Greiner; T. Kruehler; S. Larsson; R. Buehler; P. Ogle; A. Szostek; A. Berdyugin; R. Itoh; A. E. Wehrle; J. Chiang; D. Blinov; W. Max-Moerbeck; H. D. Aller; R. D. Blandford; E. Benítez; M. Yamanaka; Motoki Kino; I. Agudo; Shuji Sato; Kelly Blumenthal; Jean‐Pierre Macquart; U. Bach; Makoto Uemura; M. Villata; Takaaki Tanaka; G. Tosti; A. Rossi; E. Cavazzuti; C. M. Raiteri; M. Sikora; Mahito Sasada; Y. Fukazawa; A. C. S. Readhead; A. A. Arkharov; W. Collmar; Koji S. Kawabata; Douglas C.‐J. Bock; M. F. Aller; A. Reimer; J. L. Richards; N. Gehrels; Ł. Stawarz; Y. Uchiyama; K. Sakimoto; G. Madejski; M. Böttcher; Krzysztof Nalewajko

doi:10.1088/0004-637x/754/2/114

THE STRUCTURE AND EMISSION MODEL OF THE RELATIVISTIC JET IN THE QUASAR 3C 279 INFERRED FROM RADIO TO HIGH-ENERGY γ-RAY OBSERVATIONS IN 2008-2010

M. Hayashida(The University of Tokyo), C. S. Buemi(Osservatorio Astrofisico di Catania), S. Ciprini(Agenzia Spaziale Italiana), J. Greiner(Max Planck Institute for Extraterrestrial Physics), T. Kruehler(University of Copenhagen), S. Larsson(Karolinska Institutet), R. Buehler(Deutsches Elektronen-Synchrotron DESY), P. Ogle(Vassar College), A. Szostek(Jagiellonian University), A. Berdyugin(University of Turku), R. Itoh(Bisei Astronomical Observatory), A. E. Wehrle(California Institute of Technology), J. Chiang(SLAC National Accelerator Laboratory), D. Blinov(Institute of Applied Astronomy), W. Max-Moerbeck(University of Chile), H. D. Aller(University of Michigan), R. D. Blandford(California Institute of Technology), E. Benítez(Universidad Nacional Autónoma de México), M. Yamanaka(The University of Osaka), Motoki Kino(Kogakuin University), I. Agudo(Instituto de Astrofísica de Andalucía), Shuji Sato(Josai International University), Kelly Blumenthal(Boston University), Jean‐Pierre Macquart(Curtin University), U. Bach(Max Planck Institute for Radio Astronomy), Makoto Uemura(Hiroshima University), M. Villata(Osservatorio Astrofisico di Torino), Takaaki Tanaka(Konan University), G. Tosti(University of Perugia), A. Rossi(Thüringer Landessternwarte Tautenburg), E. Cavazzuti(Agenzia Spaziale Italiana), C. M. Raiteri(Osservatorio Astrofisico di Torino), M. Sikora(Silesian University of Technology), Mahito Sasada(Hiroshima University), Y. Fukazawa(Hiroshima University), A. C. S. Readhead(California Institute of Technology), A. A. Arkharov(Pulkovo Observatory), W. Collmar(Max Planck Institute for Extraterrestrial Physics), Koji S. Kawabata(Hiroshima University), Douglas C.‐J. Bock(Commonwealth Scientific and Industrial Research Organisation), M. F. Aller(University of Michigan), A. Reimer(SLAC National Accelerator Laboratory), J. L. Richards(California Institute of Technology), N. Gehrels(Goddard Space Flight Center), Ł. Stawarz(Jagiellonian University), Y. Uchiyama(Rikkyo University), K. Sakimoto(Hiroshima University), G. Madejski(Max Planck Society), M. Böttcher(North-West University), Krzysztof Nalewajko(University of Colorado Boulder)

The Astrophysical Journal

July 16, 2012

10.1088/0004-637x/754/2/114

Cited by 195

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