HAWC J2227+610 and Its Association with G106.3+2.7, a New Potential Galactic PeVatron
Department of Physics
We present the detection of very-high-energy gamma-ray emission above 100 TeV from HAWC J2227+610 with the High-Altitude Water Cherenov Gamma-Ray Observatory (HAWC) observatory. Combining our observations with previously published results by the Very Energetic Radiation Imaging Telescope Array System (VERTIAS), we interpret the gamma-ray emission from HAWC J2227+610 as emission from protons with a lower limit in their cutoff energy of 800 TeV. The most likely source of the protons is the associated supernova remnant G106.3+2.7, making it a good candidate for a Galactic PeVatron. However, a purely leptonic origin of the observed emission cannot be excluded at this time.
Astrophysical Journal Letters
HAWC J2227+610 and Its Association with G106.3+2.7, a New Potential Galactic PeVatron.
Astrophysical Journal Letters,
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