Very High Energy Gamma-ray Emission from the Binary System LS I +61 303

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    • uploaded July 8, 2021

    Discussion timeslot (ZOOM-Meeting): 16. July 2021 - 12:00
    ZOOM-Meeting URL: https://desy.zoom.us/j/98542982538
    ZOOM-Meeting ID: 98542982538
    ZOOM-Meeting Passcode: ICRC2021
    Corresponding Session: https://icrc2021-venue.desy.de/channel/50-Galactic-Compact-Objects-Pulsars-Binary-Systems-Microquasars-GAD-GAI/124
    Live-Stream URL: https://icrc2021-venue.desy.de/livestream/Discussion-04/5

    Abstract:
    'LS I +61 303 is one of around ten gamma-ray binaries detected so far, each characterized by a spectral energy distribution dominated by MeV-GeV photons. It is located at a distance of 2 kpc and consists of a compact object (black hole or neutron star) in an eccentric orbit around a 10-15

    Tags:
    Categories: Gamma Ray Indirect, Scientific Contributions
    Presenter:

    David Kieda


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