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  • Exploring the nature of a possible PeVatron/ neutrino source MGRO J1908+06

    Seminar Title  

    Exploring the nature of a possible PeVatron/ neutrino source MGRO J1908+06

       
    Speaker:   DrLI Jian
       

     Affiliation:   

     (German synchrotron center)

       
    When

    Thurseday morning, Nov.22, 10:00 a.m.

       

    Where:   

    Room 302, No.3  building , Xianlin campus (PMO, CAS)
     

                             Welcome to Attend   

     
      ( PMO Academic Committee & Academic Circulating committee)
     

      Abstract:MGRO J1908+06 is an unidentified, bright TeV source and has been proposed as one of the most likely neutrino sources and PeVatron. However, no conclusive counterpart of MGRO J1908+06 has been detected at other wavelengths, and its nature remains unknown. Possible counterparts consistent with its position and shape include the pulsar J1907+0602 and the SNR G40.5-0.5. PSR J1907+0602 is a 106.6 ms gamma-ray pulsar with high spin down power (~ 2.8×10^36 erg/s). SNR G40.5-0.5 is ~20k year old supernova remnant. By analyzing multi-wavelength data (GeV (Fermi-LAT), X-ray, optical, radio), we explore the possibility of MGRO J1908+06 being powered by a pulsar wind nebula from PSR J1907+0602 or via hadronic processes from cosmic rays produced in SNR G40.5-05.  

     
     
     
     
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