dc.contributor.author | Lang, Mark | en |
dc.date.accessioned | 2011-03-23T13:29:32Z | en |
dc.date.available | 2011-03-23T13:29:32Z | en |
dc.date.issued | 2009 | en |
dc.identifier.citation | The VERITAS Collaboration, the VLBA 43 GHz M 87 Monitoring Team, the H.E.S.S. ...(2009)Radio Imaging of the Very-High-Energy Gamma-Ray Emission Region in the Central Engine of a Radio Galaxy, Science 325:444-448,2009 | en |
dc.identifier.uri | http://hdl.handle.net/10379/1770 | en |
dc.description.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. | en |
dc.format | application/pdf | en |
dc.language.iso | en | en |
dc.rights | Attribution-NonCommercial-NoDerivs 3.0 Ireland | |
dc.rights.uri | https://creativecommons.org/licenses/by-nc-nd/3.0/ie/ | |
dc.subject | Astrophysics - High Energy Astrophysical Phenomena | en |
dc.subject | Astrophysics - Galaxy Astrophysics | en |
dc.title | Radio Imaging of the Very-High-Energy Gamma-Ray Emission Region in the Central Engine of a Radio Galaxy | en |
dc.type | Article | en |
dc.local.publishedsource | http://arxiv.org/pdf/0908.0511 | en |
dc.description.peer-reviewed | peer-reviewed | en |
dc.local.authors | The VERITAS Collaboration, the VLBA 43 GHz M 87 Monitoring Team, the H.E.S.S. Collaboration, and the MAGIC Collaboration | en |
dc.local.arxivid | 0908.0511 | en |
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