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Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/51292
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dc.contributor.authorAcciari, V.-
dc.contributor.authorAliu, E.-
dc.contributor.authorArlen, T.-
dc.contributor.authorBautista, M.-
dc.contributor.authorBeilicke, M.-
dc.contributor.authorBenbow, W.-
dc.contributor.authorBradbury, S.-
dc.contributor.authorBuckley, J.-
dc.contributor.authorBugaev, V.-
dc.contributor.authorButt, Y.-
dc.contributor.authorByrum, K.-
dc.contributor.authorCannon, A.-
dc.contributor.authorCelik, O.-
dc.contributor.authorCesarini, A.-
dc.contributor.authorChow, Y.-
dc.contributor.authorCiupik, L.-
dc.contributor.authorCogan, P.-
dc.contributor.authorCui, W.-
dc.contributor.authorDickherber, R.-
dc.contributor.authorFegan, S.-
dc.contributor.authoret al.-
dc.date.issued2009-
dc.identifier.citationScience, 2009; 325(5939):444-448-
dc.identifier.issn0036-8075-
dc.identifier.issn1095-9203-
dc.identifier.urihttp://hdl.handle.net/2440/51292-
dc.description.abstractThe 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.-
dc.description.statementofresponsibilityThe VERITAS Collaboration, the VLBA 43 GHz M87 Monitoring Team, the H.E.S.S. Collaboration, the MAGIC Collaboration-
dc.language.isoen-
dc.publisherAmerican Association for the Advancement of Science-
dc.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-
dc.source.urihttp://arxiv.org/abs/0908.0511-
dc.subjectVERITAS Collaboration-
dc.subjectVLBA 43 GHz M87 Monitoring Team-
dc.subjectH.E.S.S. Collaboration-
dc.subjectMAGIC Collaboration-
dc.titleRadio imaging of the very-high-energy γ-ray emission region in the central engine of a radio galaxy-
dc.title.alternativeRadio imaging of the very-high-energy gamma-ray emission region in the central engine of a radio galaxy-
dc.typeJournal article-
dc.identifier.doi10.1126/science.1175406-
pubs.publication-statusPublished-
dc.identifier.orcidRowell, G. [0000-0002-9516-1581]-
Appears in Collections:Aurora harvest
Chemistry and Physics publications

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