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    Detection of Gamma-Ray Emission from the Vela Pulsar Wind Nebula with AGILE

    Access Status
    Fulltext not available
    Authors
    Pellizzoni, A.
    Trois, A.
    Tavani, M.
    Pilia, M.
    Giuliani, A.
    Pucella, G.
    Esposito, P.
    Sabatini, S.
    Piano, G.
    Argan, A.
    Barbiellini, G.
    Bulgarelli, A.
    Burgay, M.
    Caraveo, P.
    Cattaneo, P.
    Chen, A.
    Cocco, V.
    Contessi, T.
    Costa, E.
    D'Ammando, F.
    Del Monte, E.
    De Paris, G.
    Di Cocco, G.
    Di Persio, G.
    Donnarumma, I.
    Evangelista, Y.
    Feroc, M.
    Ferrari, A.
    Fiorini, M.
    Fuschino, F.
    Galli, M.
    Gianotti, F.
    Hotan, Aidan
    Labanti, C.
    Lapshov, I.
    Lazzarotto, F.
    Lipari, P.
    Longo, F.
    Marisaldi, M.
    Mastropietro, M.
    Mereghetti, S.
    Moretti, E.
    Morselli, A.
    Pacciani, L.
    Palfreyman, J.
    Perotti, F.
    Picozza, P.
    Pittori, C.
    Possenti, A.
    Prest, M.
    Rapisarda, M.
    Rappoldi, A.
    Rossi, E.
    Rubini, A.
    Santolamazza, P.
    Scalise, E.
    Soffitta, P.
    Striani, E.
    Trifoglio, M.
    Vallazza, E.
    Vercellone, S.
    Verrecchia, F.
    Vittorini, V.
    Zambra, A.
    Zanello, D.
    Giommi, P.
    Colafrancesco, S.
    Antonelli, A.
    Salotti, L.
    D’Amico, N.
    Bignami, G.F.
    Date
    2010
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Pellizzoni, A. and Trois, A. and Tavani, M. and Pilia, M. and Giuliani, A. and Pucella, G. and Esposito, P. et al. 2010. Detection of Gamma-Ray Emission from the Vela Pulsar Wind Nebula with AGILE. Science. 327 (5966): pp. 663-665.
    Source Title
    Science
    DOI
    10.1126/science.1183844
    ISSN
    00368075
    School
    Department of Imaging and Applied Physics
    URI
    http://hdl.handle.net/20.500.11937/48241
    Collection
    • Curtin Research Publications
    Abstract

    Pulsars are known to power winds of relativistic particles that can produce bright nebulae by interacting with the surrounding medium. These pulsar wind nebulae (PWNe) are observed in the radio, optical, x-rays and, in some cases, also at TeV energies, but the lack of information in the gamma-ray band prevents from drawing a comprehensive multiwavelength picture of their phenomenology and emission mechanisms. Using data from the AGILE satellite, we detected the Vela pulsar wind nebula in the energy range from 100 MeV to 3 GeV. This result constrains the particle population responsible for the GeV emission, probing multivavelength PWN models, and establishes a class of gamma-ray emitters that could account for a fraction of the unidentified Galactic gamma-ray sources.

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