%0 Journal Article
%T Discovery of very high energy gamma-rays associated with an X-ray binary
%+ AstroParticule et Cosmologie (APC (UMR_7164))
%+ Laboratoire de Physique Théorique et Astroparticules (LPTA)
%+ Laboratoire Leprince-Ringuet (LLR)
%+ Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE)
%A Aharonian, F.
%A Akhperjanian, A.G.
%A Aye, K.-M.
%A Bazer-Bachi, A.R.
%A Beilicke, M.
%A Benbow, W.
%A Berge, D.
%A Berghaus, P.
%A Bernlöhr, K.
%A Boisson, C.
%A Bolz, O.
%A Borrel, V.
%A Braun, I.
%A Breitling, F.
%A Brown, A.M.
%A Bussons Gordo, J.
%A Chadwick, P.M.
%A Chounet, L.-M.
%A Cornils, R.
%A Costamante, L.
%A Degrange, B.
%A Dickinson, H.J.
%A Djannati-Ataï, A.
%A Drury, L.O'C.
%A Dubus, G.
%A Emmanoulopoulos, D.
%A Espigat, P.
%A Feinstein, F.
%A Fleury, P.
%A Fontaine, G.
%A Fuchs, Y.
%A Funk, S.
%A Gallant, Y.A.
%A Giebels, B.
%A Gillessen, S.
%A Glicenstein, J.F.
%A Goret, P.
%A Hadjichristidis, C.
%A Hauser, M.
%A Heinzelmann, G.
%A Henri, G.
%A Hermann, G.
%A Hinton, J.A.
%A Hofmann, W.
%A Holleran, M.
%A Horns, D.
%A Jacholkowska, A.
%A de Jager, O.C.
%A Khélifi, B.
%A Komin, Nu.
%A Konopelko, A.
%A Latham, I.J.
%A Le Gallou, R.
%A Lemière, A.
%A Lemoine-Goumard, M.
%A Leroy, N.
%A Lohse, T.
%A Marcowith, A.
%A Martin, J.-M.
%A Martineau-Huynh, O.
%A Masterson, C.
%A Mccomb, T.J.L.
%A de Naurois, M.
%A Nolan, S.J.
%A Noutsos, A.
%A Orford, K.J.
%A Osborne, J.L.
%A Ouchrif, M.
%A Panter, M.
%A Pelletier, G.
%A Pita, S.
%A Pühlhofer, G.
%A Punch, M.
%A Raubenheimer, B.C.
%A Raue, M.
%A Raux, J.
%A Rayner, S.M.
%A Reimer, A.
%A Reimer, O.
%A Ripken, J.
%A Rob, L.
%A Rolland, L.
%A Rowell, G.
%A Sahakian, V.
%A Saugé, L.
%A Schlenker, S.
%A Schlickeiser, R.
%A Schuster, C.
%A Schwanke, U.
%A Siewert, M.
%A Sol, H.
%A Spangler, D.
%A Steenkamp, R.
%A Stegmann, C.
%A Tavernet, J.-P.
%A Terrier, R.
%A Théoret, C.G.
%A Tluczykont, M.
%A Vasileiadis, G.
%A Venter, C.
%A Vincent, P.
%A Völk, H.J.
%A Wagner, S.J.
%< avec comité de lecture
%Z APC-05-25;PTA/05-34
%@ 0036-8075
%J Science
%I American Association for the Advancement of Science (AAAS)
%V 309
%P 746-749
%8 2005
%D 2005
%Z astro-ph/0508298
%Z Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
%Z Sciences of the Universe [physics]/Astrophysics [astro-ph]Journal articles
%X X-ray binaries are composed of a normal star in orbit around a neutron star or stellar-mass black hole. Radio and X-ray observations have led to the presumption that some X-ray binaries called microquasars behave as scaled down active galactic nuclei. Microquasars have resolved radio emission that is thought to arise from a relativistic outflow akin to active galactic nuclei jets, in which particles can be accelerated to large energies. Very high energy gamma-rays produced by the interactions of these particles have been observed from several active galactic nuclei. Using the High Energy Stereoscopic System, we find evidence for gamma-ray emission >100 GeV from a candidate microquasar, LS 5039, showing that particles are also accelerated to very high energies in these systems.
%G English
%Z HESS
%L in2p3-00024532
%U https://hal.in2p3.fr/in2p3-00024532
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%~ OBSPM
%~ CEA
%~ UNIV-PARIS7
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%~ UPMC
%~ LPTA
%~ LLR
%~ LPNHE
%~ APC
%~ CNRS
%~ UNIV-MONTP2
%~ X-LLR
%~ X-DEP
%~ X-DEP-PHYS
%~ DSM-IRFU
%~ IRFU-APC
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