Speaker
Mr
Yiwei Bao
(Nanjing University)
Description
Multi-wavelength observations indicate that there must be a hadronic component in the $\gamma$-ray spectrum of SNR G106.3+2.7. However, fitting the hard $\gamma$-ray spectrum requires a hard proton spectrum, while usual observations and recent numerical simulations prefer a soft proton
spectrum. Here we explore an alternative scenario to explain the γ-ray spectrum
of G106.3+2.7 within the current understanding of acceleration and escape processes.
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Primary author
Mr
Yiwei Bao
(Nanjing University)
Co-author
Dr
Yang Chen
(Department of Astronomy, Nanjing University)
