%0 Conference Proceedings
%T H.E.S.S. observation of the Vela X nebula
%+ Laboratoire d'Annecy de Physique des Particules (LAPP)
%+ Laboratoire de Physique Théorique et Astroparticules (LPTA)
%+ Laboratoire Leprince-Ringuet (LLR)
%A Dubois, F.
%A Glück, B.
%A C. de Jager, O.
%A Gallant, Y.
%A Hinton, J.
%A Khélifi, B.
%A Lamanna, G.
%A Stegmann, C.
%< avec comité de lecture
%Z LAPP-EXP-2009-17
%( Proceedings of the 31st International Cosmic Ray Conference
%B 31st International Cosmic Ray Conference (ICRC 2009)
%C Lodz, Poland
%V A paraître
%8 2009-07-07
%D 2009
%Z Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
%Z Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Conference papers
%X Vela X is one of the nearest Pulsar Wind Nebulae (PWN) and has served as prototype for evolutionary studies. Associated with the pulsar B0833-45, Vela X has been observed at different wavelengths and in particular in and X-ray bands. The H.E.S.S. Cherenkov telescope array has observed Vela X in 2004 and 2005, discovering very high energy gamma-ray emission in this region, centered to the south of the pulsar, and contained within a region of 0.8 degrees radius. Additional observations from 2006 to 2009 allowed further investigation into the Vela X non-thermal emission. In this work the latest results on the Vela X gamma-ray emission are presented in the context of a multiwave-length analysis.
%G English
%Z HESS
%2 https://hal.in2p3.fr/in2p3-00461297/document
%2 https://hal.in2p3.fr/in2p3-00461297/file/icrc0641.pdf
%L in2p3-00461297
%U https://hal.in2p3.fr/in2p3-00461297
%~ IN2P3
%~ X
%~ UNIV-SAVOIE
%~ UGA
%~ LPTA
%~ LAPP
%~ LLR
%~ CNRS
%~ UNIV-MONTP2
%~ X-LLR
%~ X-DEP
%~ X-DEP-PHYS
%~ UNIV-MONTPELLIER
%~ USMB-COMUE
%~ UM1-UM2