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000139880 005__ 20250730162606.0
000139880 0247_ $$2arXiv$$aarXiv:1111.5341
000139880 0247_ $$2doi$$a10.1088/0004-637X/746/2/151
000139880 0247_ $$2altmetric$$aaltmetric:467197
000139880 0247_ $$2inspire$$ainspire:955117
000139880 0247_ $$2WOS$$aWOS:000300406300037
000139880 0247_ $$2openalex$$aopenalex:W2141145035
000139880 037__ $$aPHPPUBDB-23324
000139880 041__ $$aEnglish
000139880 082__ $$a520
000139880 0881_ $$aarXiv:1111.5341
000139880 088__ $$2arXiv$$aarXiv:1111.5341
000139880 1001_ $$aAbramowski, A.$$b0
000139880 1101_ $$aDESY$$bStandort Zeuthen
000139880 245__ $$aThe 2010 very high energy gamma-ray flare and 10 years of multi-wavelength observations of M 87
000139880 260__ $$aChicago, Ill. [u.a.]$$bUniv.11032$$c2012
000139880 300__ $$a151
000139880 3367_ $$2DRIVER$$aarticle
000139880 3367_ $$2DataCite$$aOutput Types/Journal article
000139880 3367_ $$0PUB:(DE-HGF)29$$2PUB:(DE-HGF)$$aReport$$mreport
000139880 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1521034328_26390
000139880 3367_ $$2BibTeX$$aARTICLE
000139880 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000139880 3367_ $$00$$2EndNote$$aJournal Article
000139880 440_0 $$0PERI:(DE-600)1473835-1$$aAstrophys. J.$$v746$$x0004-637X
000139880 500__ $$3Converted on 2013-05-30 09:34$$a19 pages, 5 figures; Corresponding authors: M. Raue, L. Stawarz, D. Mazin, P. Colin, C. M. Hui, M. Beilicke; Fig. 1 lightcurve data available online: http://www.desy.de/~mraue/m87/
000139880 500__ $$3Converted on 2013-06-21 19:21
000139880 520__ $$aAbridged: The giant radio galaxy M 87 with its proximity, famous jet, and very massive black hole provides a unique opportunity to investigate the origin of very high energy (VHE; E>100 GeV) gamma-ray emission generated in relativistic outflows and the surroundings of super-massive black holes. M 87 has been established as a VHE gamma-ray emitter since 2006. The VHE gamma-ray emission displays strong variability on timescales as short as a day. In this paper, results from a joint VHE monitoring campaign on M 87 by the MAGIC and VERITAS instruments in 2010 are reported. During the campaign, a flare at VHE was detected triggering further observations at VHE (H.E.S.S.), X-rays (Chandra), and radio (43 GHz VLBA). The excellent sampling of the VHE gamma-ray light curve enables one to derive a precise temporal characterization of the flare: the single, isolated flare is well described by a two-sided exponential function with significantly different flux rise and decay times. While the overall variability pattern of the 2010 flare appears somewhat different from that of previous VHE flares in 2005 and 2008, they share very similar timescales (~day), peak fluxes (Phi(>0.35 TeV) ~= (1-3) x 10^-11 ph cm^-2 s^-1), and VHE spectra. 43 GHz VLBA radio observations of the inner jet regions indicate no enhanced flux in 2010 in contrast to observations in 2008, where an increase of the radio flux of the innermost core regions coincided with a VHE flare. On the other hand, Chandra X-ray observations taken ~3 days after the peak of the VHE gamma-ray emission reveal an enhanced flux from the core. The long-term (2001-2010) multi-wavelength light curve of M 87, spanning from radio to VHE and including data from HST, LT, VLA and EVN, is used to further investigate the origin of the VHE gamma-ray emission. No unique, common MWL signature of the three VHE flares has been identified.
000139880 536__ $$0G:(DE-HGF)POF2-52x$$a52x - Programm Astroteilchenphysik - Topic unbekannt (POF2-52x)$$cPOF2-52x$$fPOF II$$x0
000139880 588__ $$aDataset connected to CrossRef, INSPIRE
000139880 650_7 $$2INSPIRE$$agamma ray: VHE
000139880 650_7 $$2INSPIRE$$agamma ray: emission
000139880 650_7 $$2INSPIRE$$atime dependence
000139880 650_7 $$2INSPIRE$$agalaxy: radio wave
000139880 650_7 $$2INSPIRE$$agamma ray: flux
000139880 650_7 $$2INSPIRE$$ablack hole
000139880 650_7 $$2INSPIRE$$aVERITAS
000139880 650_7 $$2INSPIRE$$aMAGIC
000139880 650_7 $$2INSPIRE$$aHESS
000139880 650_7 $$2INSPIRE$$aX-ray: flux
000139880 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0
000139880 7001_ $$aAcero, F.$$b1
000139880 7001_ $$aAharonian, F.$$b2
000139880 7001_ $$aAkhperjanian, A. G.$$b3
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000139880 7001_ $$aBalzer, A.$$b5
000139880 7001_ $$aBarnacka, A.$$b6
000139880 7001_ $$aBarres de Almeida, U.$$b7
000139880 7001_ $$aBecherini, Y.$$b8
000139880 7001_ $$aBecker, J.$$b9
000139880 7001_ $$aBehera, B.$$b10
000139880 7001_ $$aBernlohr, K.$$b11
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