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Radio imaging of the very-high-energy γ-ray emission region in the central engine of a radio galaxy

  • V. A. Acciari
  • , E. Aliu
  • , T. Arlen
  • , M. Bautista
  • , M. Beilicke
  • , W. Benbow
  • , S. M. Bradbury
  • , J. H. Buckley
  • , V. Bugaev
  • , Y. Butt
  • , K. Byrum
  • , A. Cannon
  • , O. Celik
  • , A. Cesarini
  • , Y. C. Chow
  • , L. Ciupik
  • , P. Cogan
  • , W. Cui
  • , R. Dickherber
  • , S. J. Fegan
  • J. P. Finley, P. Fortin, L. Fortson, A. Fumiss, D. Gall, G. H. Gillanders, J. Grube, R. Guenette, G. Gyuk, D. Hanna, J. Holder, D. Horan, C. M. Hui, T. B. Humensky, A. Imran, P. Kaaret, N. Karlsson, D. Kieda, J. Kildea, A. Konopelko, H. Krawczynski, F. Krennrich, M. J. Lang, S. LeBohec, G. Maier, A. McCann, M. McCutcheon, J. Millis, P. Moriarty, R. A. Ong, A. N. Otte, D. Pandel, J. S. Perkins, D. Petry, M. Pohl, J. Quinn, K. Ragan, L. C. Reyes, P. T. Reynolds, E. Roache, E. Roache, H. J. Rose, M. Schroedter, G. H. Sembroski, A. W. Smith, S. P. Swordy, M. Theiling, J. A. Toner, A. Varlotta, S. Vincent, S. P. Wakely, J. E. Ward, T. C. Weekes, A. Weinstein, D. A. Williams, S. Wissel, M. Wood, R. C. Waiker, F. Davies, P. E. Hardee, W. Junor, C. Ly, F. Aharonian, A. G. Akhperjanian, G. Anton, U. Barres De Almeida, A. R. Bazer-Bachi, Y. Becherini, B. Behera, K. Bemlöhr, A. Bochow, C. Boisson, J. Bolmont, V. Borrel, J. Brucker, F. Brun, P. Brun, R. Bühler, T. Bulik, I. Büsching, T. Boutelier, P. M. Chadwick, A. Charbonnier, R. C.G. Chaves, A. Cheesebrough, L. M. Chounet, A. C. Clapson, G. Coignet, M. Dalton, M. K. Daniel, I. D. Davids, B. Degrange, C. Deil, H. J. Dickinson, A. Djannati-Ataï, W. Domainko, L. O. Drury, F. Dubois, G. Dubus, J. Dyks, M. Dyrda, K. Egberts, D. Emmanoutopoulos, P. Espigat, C. Famier, F. Feinstein, A. Fiasson, A. Förster, G. Fontaine, M. Füßling, S. Gabici, Y. A. Gallant, L. Gérard, D. Gerbig, B. Giebels, J. F. Glicenstein, B. Glück, P. Goret, D. Göhring, D. Hauser, M. Hauser, S. Heinz, G. Heinzelmann, G. Henri, G. Hermann, J. A. Hinton, A. Hoffmann, W. Hofmann, M. Holleran, S. Hoppe, D. Horns, A. Jacholkowska, O. C. De Jager, C. Jahn, I. Jung, K. Katarzyriski, U. Katz, S. Kaufmann, E. Kendziorra, M. Kerschhaggl, D. Khangulyan, B. Khélifi, D. Keogh, W. Klužniak, T. Kneiske, Nu Kbmin, K. Kosack, G. Lamanna, J. P. Lenain, T. Lohse, V. Marandon, J. M. Martin, O. Martineau-Huynh, A. Marcowith, D. Maurin, T. J.L. McComb, M. C. Medina, R. Moderski, E. Moulin, M. Naumann-Godo, M. De Naurois, D. Nedbal, D. Nekrassov, B. Nicholas, J. Niemiec, S. J. Nolan, S. Ohm, J. F. Olive, E. De Oña Wilhelmi, K. J. Orford, M. Ostrowski, M. Panter, M. Paz Arribas, G. Pedaletti, G. Pelletier, P. O. Petrucci, S. Pita, G. Pûhlhofer, M. Punch, A. Quirrenbach, B. C. Raubenheimer, M. Raue, S. M. Rayner, M. Renaud, F. Rieger, J. Ripken, L. Rob, S. Rosier-Lees, G. Rowell, B. Rudak, C. B. Rulten, J. Ruppel, V. Sahakian, A. Santangelo, R. Schlickeiser, F. M. Schock, R. Schröder, U. Schwanke, S. Schwarzburg, S. Schwemmer, A. Shalchi, M. Sikora, J. L. Skilton, H. Sol, D. Spangler, L. Stawarz, R. Steenkamp, C. Stegmann, F. Stinzing, G. Superina, A. Szostek, P. H. Tam, J. P. Tavemet, R. Terrier, O. Tibolla, M. Tluczykont, C. Van Eldik, G. Vasileiadis, C. Venter, L. Venter, J. P. Vialle, P. Vincent, M. Vivier, H. J. Volk, F. Volpe, S. J. Wagner, M. Ward, A. A. Zdziarski, A. Zech, H. Anderhub, L. A. Antonelli, P. Antoranz, M. Backes, C. Baixeras, S. Balestra, J. A. Barrio, D. Bastieri, J. Becerra Gonzalez, J. K. Becker, W. Bednarek, K. Berger, E. Bernardini, A. Biland, R. K. Bock, G. Bonnoli, P. Bordas, D. Borla Tridon, V. Bosch-Ramon, D. Bose, I. Braun, T. Bretz, I. Britvitch, M. Camara, E. Carmona, S. Commichau, J. L. Contreras, J. Cortina, M. T. Costado, S. Covino, V. Curtef, F. Dazzi, A. De Angelis, E. De Cea Del Pozo, C. Delgado Mendez, R. De Los Reyes, B. De Lotto, M. De Maria, F. De Sabata, A. Dominguez, D. Dorner, M. Dora, D. Elsaesser, M. Errando, D. Ferenc, E. Fernández, R. Firpo, M. V. Fonseca, L. Font, N. Galante, R. J.García López, M. Garczarczyk, M. Gaug, F. Goebel, D. Hadasch, M. Hayashida, A. Herrero, D. Hildebrand, D. Höhne-Mönch, J. Hose, C. C. Hsu, T. Jogler, D. Kranich, A. La Barbera, A. Laille, E. Leonardo, E. Lindfors, S. Lombardi, F. Longo, M. López, E. Lorenz, P. Majumdar, G. Maneva, N. Mankuzhiyil, K. Mannheim, L. Maraschi, M. Mariotti, M. Martinez, D. Mazin, M. Meucci, J. M. Miranda, R. Mirzoyan, H. Miyamoto, J. Moldón, M. Moles, A. Moraleja, D. Nieto, K. Nilsson, J. Ninkovic, I. Oya, R. Paoletti, J. M. Paredes, M. Pasanen, D. Pascoli, F. Pauss, R. G. Pegna, M. A. Perez-Torres, M. Persic, L. Peruzzo, F. Prada, E. Prandini, N. Puchades, I. Reichardt, W. Rhode, M. Ribo, J. Rico, M. Rissi, A. Robert, S. Rügamer, A. Saggion, T. Y. Salto, M. Salvati, M. Sanchez-Conde, K. Satalecka, V. Scalzotto, V. Scapin, T. Schweizer, M. Shayduk, S. N. Shore, N. Sidro, A. Sierpowska-Bartosik, A. Sillanpää, J. Sitarek, D. Sobczynska, F. Spanier, A. Stamerra, L. S. Stark, L. Takalo, F. Tavecchio, P. Temnikov, D. Tescaro, M. Teshima, D. F. Torres, N. Turini, H. Vankov, R. M. Wagner, V. Zabalza, F. Zandanel, R. Zanin, J. Zapatera
  • Center for Astrophysics | Harvard & Smithsonian
  • The Bartol Research Institute
  • University of California, Los Angeles
  • McGill University
  • Washington University in St. Louis
  • University of Leeds
  • Argonne National Laboratory
  • University College Dublin
  • IDA Business Park
  • Adler Planetarium
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  • Iowa State University
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  • Galway-Mayo Institute of Technology
  • European Southern Observatory
  • University of Chicago
  • Cork Institute of Technology
  • National Radio Astronomy Observatory Socorro
  • New Mexico Tech
  • University of Alabama
  • MST-8, Los Alamos National Laboratory
  • Max-Planck-Institut für Kernphysik
  • Dublin Institute for Advanced Studies
  • Yerevan Physics Institute
  • Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
  • Durham University
  • CNRS
  • Astroparticule and Cosmol APC
  • Landessternwarte Heidelberg
  • LUTH - Laboratoire de l'Univers et de ses Theories
  • Universités Paris VI and VII
  • Universite Paris-Saclay
  • Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences
  • North-West University
  • Division Technique
  • Ip Paris
  • Université Paris-Sud
  • HumboldtUniversität zu Berlin
  • University of Namibia
  • Lnstytut Fizyki Jadrowej PAN
  • Laboratoire Univers et Particules de Montpellier
  • Ruhr-University Bochum
  • Universität Hamburg
  • University of Tübingen
  • Nicolaus Copernicus University
  • Charles University
  • University of Adelaide
  • CNRS and Max-Planck-Gessellschaft
  • Jagiellonian University
  • ETH Zurich
  • Istituto di Astrofisica e Planetologia Spaziali (IAPS)
  • Complutense University
  • University of Dortmund
  • University of São Paulo
  • University of Padova
  • Instituto de Astrofisica de Canarias
  • University of Lodz
  • c/o DESY
  • Max-Planck-Institut für Physik
  • University of Siena
  • University of Barcelona
  • University of Würzburg
  • The Barcelona Institute of Science and Technology
  • Research Unit; CIBERNED and Universidad de La Laguna
  • and Physics University of Udine
  • University of Sheffield
  • Instituto de Astrofísica de Andalucía-CSIC
  • University of California, Davis
  • University of Turku
  • Institute for Nuclear Research and Nuclear Energy Bulgarian Academy of Sciences
  • INFN Sezione di Trieste
  • Pompeu Fabra University (UPF)
  • University of Pisa

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

239 Citations (Scopus)

Résumé

The accretion of matter onto a massive black hole is believed to feed the relativistic plasma jets found in many active galactic nuclei (AGN). Although some AGN accelerate particles to energies exceeding 1012 electron volts and are bright sources of very-high-energy (VHE) y-ray emission, it is not yet known where the VHE emission originates. Here we report on radio and VHE observations of the radio galaxy Messier 87, revealing a period of extremely strong VHE y-ray flares accompanied by a strong increase of the radio flux from its nucleus. These results imply that charged particles are accelerated to very high energies in the immediate vicinity of the black hole.

langue originaleAnglais
Pages (de - à)444-468
Nombre de pages25
journalScience
Volume325
Numéro de publication5939
Les DOIs
étatPublié - 24 juil. 2009

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