Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/51292
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Type: Journal article
Title: Radio imaging of the very-high-energy γ-ray emission region in the central engine of a radio galaxy
Other Titles: Radio imaging of the very-high-energy gamma-ray emission region in the central engine of a radio galaxy
Author: Acciari, V.
Aliu, E.
Arlen, T.
Bautista, M.
Beilicke, M.
Benbow, W.
Bradbury, S.
Buckley, J.
Bugaev, V.
Butt, Y.
Byrum, K.
Cannon, A.
Celik, O.
Cesarini, A.
Chow, Y.
Ciupik, L.
Cogan, P.
Cui, W.
Dickherber, R.
Fegan, S.
et al.
Citation: Science, 2009; 325(5939):444-448
Publisher: American Association for the Advancement of Science
Issue Date: 2009
ISSN: 0036-8075
1095-9203
Statement of
Responsibility: 
The VERITAS Collaboration, the VLBA 43 GHz M87 Monitoring Team, the H.E.S.S. Collaboration, the MAGIC Collaboration
Abstract: 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 10^12 electron Volts (eV) and are bright sources of very-high-energy (VHE) gamma-ray emission, it is not yet known where the VHE emission originates. Here we report on radio and VHE observations of the radio galaxy M87, revealing a period of extremely strong VHE gamma-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.
Keywords: VERITAS Collaboration
VLBA 43 GHz M87 Monitoring Team
H.E.S.S. Collaboration
MAGIC Collaboration
Rights: © 2009 American Association for the Advancement of Science. Submitted to Cornell University’s online archive www.arXiv.org in 2009 by Matthias Beilicke. Post-print sourced from www.arxiv.org
DOI: 10.1126/science.1175406
Published version: http://arxiv.org/abs/0908.0511
Appears in Collections:Aurora harvest
Chemistry and Physics publications

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