Potential PeVatron supernova remnant G106.3+2.7 seen in the highest-energy gamma rays

Amenomori, M; Bao, YW; Bi, XJ; Chen, D; Chen, TL; Chen, WY; Chen, X; Chen, Y; Cirennima; Cui, SW; Danzengluobu; Ding, LK; Fang, JH; Fang, K; Feng, CF; Feng, ZY; Feng, ZY; Gao, Q; Gou, QB; Guo, YQ; Guo, YY; He, HH; He, ZT; Hibino, K; Hotta, N; Hu, HB; Hu, HB; Huang, J; Jia, HY; Jiang, L; Jin, HB; Kasahara, K; Katayose, Y; Kato, C; Kato, S; Kawata, K; Kihara, W; Ko, Y; Kozai, M; Labaciren; Le, GM; Li, AF; Li, HJ; Li, WJ; Lin, YH; Liu, B; Liu, C; Liu, JS; Liu, MY; Liu, W; Lou, YQ; Lu, H; Meng, XR; Munakata, K; Nakada, H; Nakamura, Y; Nanjo, H; Nishizawa, M; Ohnishi, M; Ohura, T; Ozawa, S; Qian, XL; Qu, XB; Saito, T; Sakata, M; Sako, TK; Shao, J; Shibata, M; Shiomi, A; Sugimoto, H; Takano, W; Takita, M; Tan, YH; Tateyama, N; Torii, S; Tsuchiya, H; Udo, S; Wang, H; Wu, HR; Xue, L; Yamamoto, Y; Yang, Z; Yokoe, Y; Yuan, AF; Zhai, LM; Zhang, HM; Zhang, JL; Zhang, X; Zhang, XY; Zhang, Y; Zhang, Y; Zhang, Y; Zhao, SP; Zhaxisangzhu; Zhou, XX

Zhang, X (corresponding author), Nanjing Univ, Sch Astron & Space Sci, Nanjing, Peoples R China.; Huang, J (corresponding author), Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing, Peoples R China.; Chen, D (corresponding author), Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China.; Ohnishi, M; Sako, TK; Takita, M (corresponding author), Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba, Japan.

NATURE ASTRONOMY, ; ():

Abstract

Cosmic rays (protons and other atomic nuclei) are believed to gain energies of petaelectronvolts (PeV) and beyond at astrophysical particle accelerato......

Full Text Link