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    A search for VHE counterparts of Galactic Fermi bright sources and MeV to TeV spectral characterization

    Access Status
    Open access via publisher
    Authors
    Tam, P.
    Wagner, S.
    Tibolla, Omar
    Chaves, R.
    Date
    2010
    Type
    Journal Article
    
    Metadata
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    Citation
    Tam, P. and Wagner, S. and Tibolla, O. and Chaves, R. 2010. A search for VHE counterparts of Galactic Fermi bright sources and MeV to TeV spectral characterization. Astronomy and Astrophysics. 518: Article ID A8.
    Source Title
    Astronomy and Astrophysics
    DOI
    10.1051/0004-6361/200913717
    ISSN
    0004-6361
    URI
    http://hdl.handle.net/20.500.11937/25936
    Collection
    • Curtin Research Publications
    Abstract

    Very high-energy (VHE; E > 100 GeV) γ-rays have been detected in a wide range of astronomical objects, such as pulsar wind nebulae (PWNe), supernova remnants (SNRs), giant molecular clouds, γ-ray binaries, the Galactic center, active galactic nuclei (AGN), radio galaxies, starburst galaxies, and possibly star-forming regions. At lower energies, observations using the Large Area Telescope (LAT) onboard Fermi provide a rich set of data that can be used to study the behavior of cosmic accelerators in the MeV to TeV energy bands. In particular, the improved angular resolution of current telescopes in both bands compared to previous instruments significantly reduces source confusion and facilitates identification of associated counterparts at lower energies. In this paper, a comprehensive search for VHE γ-ray sources that are spatially coincident with Galactic Fermi/LAT bright sources is performed, and the available MeV to TeV spectra of coincident sources compared. It is found that bright LAT GeV sources are correlated with TeV sources, in contrast to previous studies using EGRET data. Moreover, a single spectral component seems unable to describe the MeV to TeV spectra of many coincident GeV/TeV sources. It has been suggested that γ-ray pulsars may be accompanied by VHE γ-ray emitting nebulae, a hypothesis that can be tested with VHE observations of these pulsars.

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