%0 Conference Proceedings
%T Radio and X-ray Observations of the Possible New Gamma-ray binary HESS J0632+057
%+ Laboratoire d'Astrophysique de Grenoble (LAOG)
%+ Laboratoire d'Annecy de Physique des Particules (LAPP)
%+ Laboratoire de Physique Théorique et Astroparticules (LPTA)
%A L. Skilton, J.
%A A. Hinton, J.
%A Brucker, J.
%A Pandey-Pommier, M.
%A C. Cheung, C.
%A A. Aharonian, F.
%A Dubus, G.
%A Fiasson, A.
%A Funk, S.
%A Gallant, Y.
%A Marcowith, A.
%A Reimer, O.
%Z http://aspbooks.org/a/volumes/retrieve?pdf=422/128.pdf&download=1
%< avec comité de lecture
%( Astronomical Society of the Pacific Conference Series
%( HIGH ENERGY PHENOMENA IN MASSIVE STARSASP Conference Series
%B High Energy Phenomena in Massive Stars Conference
%C Jaén, Spain
%Y J. Martı
%Y P.L. Luque-Escamilla
%Y J.A. Combi
%V 422
%P 128-134
%8 2009-02-02
%D 2009
%Z 2010ASPC..422..128S
%Z Physics [physics]/High Energy Physics - Experiment [hep-ex]
%Z Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
%Z Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Conference papers
%X HESS J0632+057 is one of the only point-like, unidentified TeV sources in our galaxy. The association of this source with the massive B0pe star MWC 148 has led to the suggestion that HESS J0632+057 could be a new gamma-ray binary system. Our recent X-ray observations with XMM-Newton have revealed a non-thermal, point-like source coincident with this star, further strengthening the identification of HESS J0632+057 as a high mass X-ray binary system. Here we present new Very Large Array (VLA) and Giant Metre-wave Radio Telescope (GMRT) observations towards HESS J0632+057 which reveal point-like variable emission at the location of MWC 148.
%G English
%L in2p3-00910837
%U https://hal.in2p3.fr/in2p3-00910837
%~ IN2P3
%~ INSU
%~ UNIV-SAVOIE
%~ UGA
%~ LPTA
%~ LAPP
%~ CNRS
%~ UNIV-GRENOBLE1
%~ UNIV-MONTP2
%~ OSUG
%~ LAOG
%~ UNIV-MONTPELLIER
%~ USMB-COMUE
%~ UM1-UM2