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dc.contributor.authorAcciari, V. A.
dc.contributor.authorAliu, E.
dc.contributor.authorAraya, M.
dc.contributor.authorArlen, T.
dc.contributor.authorAune, T.
dc.contributor.authorBeilicke, M.
dc.contributor.authorBenbow, W.
dc.contributor.authorBradbury, S. M.
dc.contributor.authorBuckley, J. H.
dc.contributor.authorBugaev, V.
dc.contributor.authorByrum, K.
dc.contributor.authorCannon, A.
dc.contributor.authorCesarini, A.
dc.contributor.authorCiupik, L.
dc.contributor.authorCollins-Hughes, E.
dc.contributor.authorCui, W.
dc.contributor.authorDickherber, R.
dc.contributor.authorDuke, C.
dc.contributor.authorFalcone, A.
dc.contributor.authorFinley, J. P.
dc.contributor.authorFortson, L.
dc.contributor.authorFurniss, A.
dc.contributor.authorGalante, N.
dc.contributor.authorGall, D.
dc.contributor.authorGodambe, S.
dc.contributor.authorGriffin, S.
dc.contributor.authorGuenette, R.
dc.contributor.authorGyuk, G.
dc.contributor.authorHanna, D.
dc.contributor.authorHolder, J.
dc.contributor.authorHughes, G.
dc.contributor.authorHui, C. M.
dc.contributor.authorHumensky, T. B.
dc.contributor.authorImran, A.
dc.contributor.authorKaaret, P.
dc.contributor.authorKertzman, M.
dc.contributor.authorKrawczynski, H.
dc.contributor.authorKrennrich, F.
dc.contributor.authorMadhavan, A. S.
dc.contributor.authorMaier, G.
dc.contributor.authorMajumdar, P.
dc.contributor.authorMcArthur, S.
dc.contributor.authorMoriarty, P.
dc.contributor.authorOng, R. A.
dc.contributor.authorOtte, A. N.
dc.contributor.authorPandel, D.
dc.contributor.authorPark, N.
dc.contributor.authorPerkins, J. S.
dc.contributor.authorPohl, M.
dc.contributor.authorProkoph, H.
dc.contributor.authorQuinn, J.
dc.contributor.authorRagan, K.
dc.contributor.authorReyes, L. C.
dc.contributor.authorReynolds, P. T.
dc.contributor.authorRoache, E.
dc.contributor.authorRose, H. J.
dc.contributor.authorSaxon, D. B.
dc.contributor.authorSembroski, G. H.
dc.contributor.authorŞentürk, G. D.
dc.contributor.authorSmith, A. W.
dc.contributor.authorTešić, G.
dc.contributor.authorTheiling, M.
dc.contributor.authorThibadeau, S.
dc.contributor.authorVarlotta, A.
dc.contributor.authorVincent, S.
dc.contributor.authorVivier, M.
dc.contributor.authorWakely, S. P.
dc.contributor.authorWard, J. E.
dc.contributor.authorWeekes, T. C.
dc.contributor.authorWeinstein, A.
dc.contributor.authorWeisgarber, T.
dc.contributor.authorWeng, S.
dc.contributor.authorWilliams, D. A.
dc.contributor.authorWood, M.
dc.contributor.authorZitzer, B.
dc.date.accessioned2018-09-20T15:58:42Z
dc.date.available2018-09-20T15:58:42Z
dc.date.issued2011-05-11
dc.identifier.citationAcciari, V. A. Aliu, E.; Araya, M.; Arlen, T.; Aune, T.; Beilicke, M.; Benbow, W.; Bradbury, S. M.; Buckley, J. H.; Bugaev, V.; Byrum, K.; Cannon, A.; Cesarini, A.; Ciupik, L.; Collins-Hughes, E.; Cui, W.; Dickherber, R.; Duke, C.; Falcone, A.; Finley, J. P.; Fortson, L.; Furniss, A.; Galante, N.; Gall, D.; Godambe, S.; Griffin, S.; Guenette, R.; Gyuk, G.; Hanna, D.; Holder, J.; Hughes, G.; Hui, C. M.; Humensky, T. B.; Imran, A.; Kaaret, P.; Kertzman, M.; Krawczynski, H.; Krennrich, F.; Madhavan, A. S.; Maier, G.; Majumdar, P.; McArthur, S.; Moriarty, P.; Ong, R. A.; Otte, A. N.; Pandel, D.; Park, N.; Perkins, J. S.; Pohl, M.; Prokoph, H.; Quinn, J.; Ragan, K.; Reyes, L. C.; Reynolds, P. T.; Roache, E.; Rose, H. J.; Saxon, D. B.; Sembroski, G. H.; Şentürk, G. D.; Smith, A. W.; Tešić, G.; Theiling, M.; Thibadeau, S.; Varlotta, A.; Vincent, S.; Vivier, M.; Wakely, S. P.; Ward, J. E.; Weekes, T. C.; Weinstein, A.; Weisgarber, T.; Weng, S.; Williams, D. A.; Wood, M.; Zitzer, B. (2011). Gamma-ray observations of the be/pulsar binary 1a 0535+262 during a giant x-ray outburst. The Astrophysical Journal 733 (2),
dc.identifier.issn0004-637X,1538-4357
dc.identifier.urihttp://hdl.handle.net/10379/10090
dc.description.abstractGiant X-ray outbursts, with luminosities of about 10(37) erg s(-1), are observed roughly every five years from the nearby Be/pulsar binary 1A 0535+262. In this article, we present observations of the source with VERITAS at very high energies (VHEs; E > 100 GeV) triggered by the X-ray outburst in 2009 December. The observations started shortly after the onset of the outburst and provided comprehensive coverage of the episode, as well as the 111 day binary orbit. No VHE emission is evident at any time. We also examined data from the contemporaneous observations of 1A 0535+262 with the Fermi/Large Area Telescope at high-energy photons (E > 0.1 GeV) and failed to detect the source at GeV energies. The X-ray continua measured with the Swift/X-Ray Telescope and the RXTE/PCA can be well described by the combination of blackbody and Comptonized emission from thermal electrons. Therefore, the gamma-ray and X-ray observations suggest the absence of a significant population of non-thermal particles in the system. This distinguishes 1A 0535+262 from those Be X-ray binaries (such as PSR B1259-63 and LS I +61 degrees 303) that have been detected at GeV-TeV energies. We discuss the implications of the results on theoretical models.
dc.publisherIOP Publishing
dc.relation.ispartofThe Astrophysical Journal
dc.subjectacceleration of particles
dc.subjectbinaries: general
dc.subjectgamma rays: general
dc.subjectstars: individual (1a 0535+262)
dc.subjectlarge-area telescope
dc.subjectproportional counter array
dc.subjecthess j0632+057
dc.subjectemission
dc.subjecta0535+262
dc.subjectcatalog
dc.subjectpulsar
dc.subjectperiod
dc.subjectcalibration
dc.subjecta-0535+26
dc.titleGamma-ray observations of the be/pulsar binary 1a 0535+262 during a giant x-ray outburst
dc.typeArticle
dc.identifier.doi10.1088/0004-637x/733/2/96
dc.local.publishedsourcehttp://iopscience.iop.org/article/10.1088/0004-637X/733/2/96/pdf
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