Explaining the gamma rays from MGRO J1908+06
Abstract
Known as one of the most brightest $\gamma$-ray sources, MGRO J1908+06 has been intensely studied for years. However, the origin of the $\gamma$-rays is still under debate. Considering hadronic contribution from the northern supernova remnant G40.5-0.5 and leptonic contribution from the southern pulsar wind of PSR J1907+0602, we present an explanation for the spectral properties (with published data from HESS, VERITAS, Milagro, and Fermi-LAT) of this source.
- Publication:
-
43rd COSPAR Scientific Assembly. Held 28 January - 4 February
- Pub Date:
- January 2021
- Bibcode:
- 2021cosp...43E1484B