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Gamma-Ray Emission from SNR W44 by CH1253 is a document available to read on EtoBox.
Most plausible explanation is that p0 particle decays are responsible for the gamma-ray emission from the supernova remnant W44, although bremsstrahlung cannot be completely ruled out. A spectral break is needed around 10 GeV/c to fit the Fermi LAT spectrum with p0 decay emission. Particle escape from the acceleration sites, the SNR shells, can explain the spectral break. The Fermi LAT data demonstrates the capability to study particle escape from SNR shells, the evolution of SNR shocks over time, and the i
- Author
- CH1253
- Language
- EN