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

dc.contributor.authorAntoranz Canales, Pedro
dc.contributor.authorBarrio Uña, Juan Abel
dc.contributor.authorContreras González, José Luis
dc.contributor.authorFonseca González, María Victoria
dc.contributor.authorMiranda Pantoja, José Miguel
dc.contributor.authorNieto Castaño, Daniel
dc.date.accessioned2023-06-20T03:35:03Z
dc.date.available2023-06-20T03:35:03Z
dc.date.issued2009-07-24
dc.description© Science. This work was also supported by ETH research grant TH 34/043, the Polish MniSzW grant N N203 390834, and the Young Investigators Program of the Helmholtz Gemeinschaft. VERITAS: This research is supported by grants from the U.S. Department of Energy, NSF, the Smithsonian Institution, the Natural Sciences and Engineering Research Council of Canada, Science Foundation Ireland, and the STFC in the U.K. We acknowledge the excellent work of the technical support staff at the Fred Lawrence Whipple Observatory and the collaborating institutions in the construction and operation of the instrument. VLBA: The Very Long Baseline Array is operated by the National Radio Astronomy Observatory, a facility of NSF, operated under cooperative agreement by Associated Universities, Inc.
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 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 Messier 87, 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.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipETH
dc.description.sponsorshipPolish MniSzW
dc.description.sponsorshipYoung Investigators Program of the Helmholtz Gemeinschaft
dc.description.sponsorshipU.S. Department of Energy
dc.description.sponsorshipNSF
dc.description.sponsorshipSmithsonian Institution
dc.description.sponsorshipNatural Sciences and Engineering Research Council of Canada
dc.description.sponsorshipScience Foundation Ireland
dc.description.sponsorshipSTFC, U.K
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/22725
dc.identifier.doi10.1126/science.1175406
dc.identifier.issn0036-8075
dc.identifier.officialurlhttp://dx.doi.org/10.1126/science.1175406
dc.identifier.relatedurlhttp://arxiv.org/abs/0908.0511
dc.identifier.urihttps://hdl.handle.net/20.500.14352/43956
dc.issue.number5939
dc.journal.titleScience
dc.language.isoeng
dc.page.final448
dc.page.initial444
dc.publisherAmer Assoc Advancement Science
dc.relation.projectIDTH 34/043
dc.relation.projectIDN N203 390834
dc.rights.accessRightsopen access
dc.subject.cdu537
dc.subject.cdu539.1
dc.subject.keywordSupermassive Black-Hole
dc.subject.keywordM87 Jet
dc.subject.keywordTEV Emission
dc.subject.keywordCrab-Nebula
dc.subject.keywordInner Jet
dc.subject.keywordVariability
dc.subject.keywordTelescope
dc.subject.keywordOutburst
dc.subject.keywordNucleus
dc.subject.keywordVeritas.
dc.subject.ucmElectrónica (Física)
dc.subject.ucmElectricidad
dc.subject.ucmFísica nuclear
dc.subject.unesco2202.03 Electricidad
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleRadio imaging of the very-high-energy gamma-ray emission region in the central engine of a radio galaxy
dc.typejournal article
dc.volume.number325
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