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  • High Energy Emission from Gamma-ray Binaries


    Seminar Title  

    High Energy Emission from Gamma-ray Binaries

    Speaker:   Prof Kwong Sang Cheng


     (The University of Hong Kong)
    When Tuesday morning, May 9, 9:30 a.m


    Room 212, Astronomy Building

                             Welcome to Attend   

      ( PMO Academic Committee & Academic Circulating committee)

       Abstract:  Gamma-ray binaries is a binary system consisting of a compact object and a massive star. Currently 7 such systems are found. They share very common features, for examples they are all detected in KeV, GeV and TeV energy range. However these emissions are not all detected in same orbital phases. In this talk we review the observed properties of these systems and explain some of these system emission properties by a unified theoretical model.

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