NAOC Open IR
Gamma-Ray Observation of the Cygnus Region in the 100-TeV Energy Region
Amenomori, M.1; Bao, Y. W.2; Bi, X. J.3; Chen, D.4; Chen, T. L.5; Chen, W. Y.3; Chen, Xu3; Chen, Y.2; Cirennima5; Cui, S. W.6; Danzengluobu5; Ding, L. K.3; Fang, J. H.3,7; Fang, K.3; Feng, C. F.8,9; Feng, Zhaoyang3; Feng, Z. Y.10; Gao, Qi5; Gomi, A.11; Gou, Q. B.3; Guo, Y. Q.3; Guo, Y. Y.3; He, H. H.3; He, Z. T.6; Hibino, K.12; Hotta, N.13; Hu, Haibing5; Hu, H. B.3; Huang, J.3; Jia, H. Y.10; Jiang, L.3; Jiang, P.4; Jin, H. B.4; Kasahara, K.14; Katayose, Y.11; Kato, C.15; Kato, S.16; Kawata, K.16; Kozai, M.17; Kurashige, D.11; Labaciren5; Le, G. M.18; Li, A. F.3,8,9,19; Li, H. J.5; Li, W. J.3,10; Li, Y.4; Lin, Y. H.3,7; Liu, B.20; Liu, C.3; Liu, J. S.3; Liu, L. Y.4; Liu, M. Y.5; Liu, W.3; Liu, X. L.4; Lou, Y-Q21,22,23,24; Lu, H.3; Meng, X. R.5; Munakata, K.15; Nakada, H.11; Nakamura, Y.3,16; Nakazawa, Y.25; Nanjo, H.1; Ning, C. C.5; Nishizawa, M.26; Ohnishi, M.16; Ohura, T.11; Okukawa, S.11; Ozawa, S.27; Qian, L.4; Qian, X.4; Qian, X. L.28; Qu, X. B.29; Saito, T.30; Sakata, M.31; Sako, T.16; Sako, T. K.16; Shao, J.3,8,9; Shibata, M.11; Shiomi, A.25; Sugimoto, H.32; Takano, W.12; Takita, M.16; Tan, Y. H.3; Tateyama, N.12; Torii, S.33; Tsuchiya, H.34; Udo, S.12; Wang, H.3; Wang, Y. P.5; Wangdui5; Wu, H. R.3; Wu, Q.5; Xu, J. L.4; Xue, L.8,9; Yamamoto, Y.31; Yang, Z.3; Yao, Y. Q.4; Yin, J.4; Yokoe, Y.16; Yu, N. P.4; Yuan, A. F.5; Zhai, L. M.4; Zhang, C. P.4; Zhang, H. M.3; Zhang, J. L.3; Zhang, X.2; Zhang, X. Y.8,9; Zhang, Y.3; Zhang, Yi35; Zhang, Ying3; Zhao, S. P.3; Zhaxisangzhu5; Zhou, X. X.10
2021-07-16
Source PublicationPHYSICAL REVIEW LETTERS
ISSN0031-9007
Volume127Issue:3Pages:6
AbstractWe report observations of gamma-ray emissions with energies in the 100-TeV energy region from the Cygnus region in our Galaxy. Two sources are significantly detected in the directions of the Cygnus OB1 and OB2 associations. Based on their positional coincidences, we associate one with a pulsar PSR J2032 + 4127 and the other mainly with a pulsar wind nebula PWN G75.2 + 0.1, with the pulsar moving away from its original birthplace situated around the centroid of the observed gamma-ray emission. This work would stimulate further studies of particle acceleration mechanisms at these gamma-ray sources.
Funding OrganizationMinistry of Science and Technology of China ; Ministry of Science and Technology of China ; Ministry of Foreign Affairs of Japan ; Ministry of Foreign Affairs of Japan ; Ministry of Education, Culture, Sports, Science and Technology ; Ministry of Education, Culture, Sports, Science and Technology ; Japan Society for the Promotion of Science in Japan ; Japan Society for the Promotion of Science in Japan ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Institute for Cosmic Ray Research (ICRR) ; Institute for Cosmic Ray Research (ICRR) ; University of Tokyo ; University of Tokyo ; Ministry of Science and Technology of China ; Ministry of Science and Technology of China ; Ministry of Foreign Affairs of Japan ; Ministry of Foreign Affairs of Japan ; Ministry of Education, Culture, Sports, Science and Technology ; Ministry of Education, Culture, Sports, Science and Technology ; Japan Society for the Promotion of Science in Japan ; Japan Society for the Promotion of Science in Japan ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Institute for Cosmic Ray Research (ICRR) ; Institute for Cosmic Ray Research (ICRR) ; University of Tokyo ; University of Tokyo ; Ministry of Science and Technology of China ; Ministry of Science and Technology of China ; Ministry of Foreign Affairs of Japan ; Ministry of Foreign Affairs of Japan ; Ministry of Education, Culture, Sports, Science and Technology ; Ministry of Education, Culture, Sports, Science and Technology ; Japan Society for the Promotion of Science in Japan ; Japan Society for the Promotion of Science in Japan ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Institute for Cosmic Ray Research (ICRR) ; Institute for Cosmic Ray Research (ICRR) ; University of Tokyo ; University of Tokyo ; Ministry of Science and Technology of China ; Ministry of Science and Technology of China ; Ministry of Foreign Affairs of Japan ; Ministry of Foreign Affairs of Japan ; Ministry of Education, Culture, Sports, Science and Technology ; Ministry of Education, Culture, Sports, Science and Technology ; Japan Society for the Promotion of Science in Japan ; Japan Society for the Promotion of Science in Japan ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Institute for Cosmic Ray Research (ICRR) ; Institute for Cosmic Ray Research (ICRR) ; University of Tokyo ; University of Tokyo
DOI10.1103/PhysRevLett.127.031102
WOS KeywordSOURCE TEV J2032+4130 ; PSR J2021+3651 ; X-RAY ; GALACTIC PLANE ; STAR-FORMATION ; EMISSION ; FERMI ; CATALOG ; SEARCH ; NEBULA
Language英语
Funding ProjectMinistry of Science and Technology of China ; Ministry of Foreign Affairs of Japan ; Ministry of Education, Culture, Sports, Science and Technology ; Japan Society for the Promotion of Science in Japan ; National Key R&D Program of China[2016YFE0125500] ; National Natural Science Foundation of China[11533007] ; National Natural Science Foundation of China[11673041] ; National Natural Science Foundation of China[11873065] ; National Natural Science Foundation of China[11773019] ; National Natural Science Foundation of China[11773014] ; National Natural Science Foundation of China[11633007] ; National Natural Science Foundation of China[11803011] ; National Natural Science Foundation of China[11851305] ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Institute for Cosmic Ray Research (ICRR) ; University of Tokyo
Funding OrganizationMinistry of Science and Technology of China ; Ministry of Science and Technology of China ; Ministry of Foreign Affairs of Japan ; Ministry of Foreign Affairs of Japan ; Ministry of Education, Culture, Sports, Science and Technology ; Ministry of Education, Culture, Sports, Science and Technology ; Japan Society for the Promotion of Science in Japan ; Japan Society for the Promotion of Science in Japan ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Institute for Cosmic Ray Research (ICRR) ; Institute for Cosmic Ray Research (ICRR) ; University of Tokyo ; University of Tokyo ; Ministry of Science and Technology of China ; Ministry of Science and Technology of China ; Ministry of Foreign Affairs of Japan ; Ministry of Foreign Affairs of Japan ; Ministry of Education, Culture, Sports, Science and Technology ; Ministry of Education, Culture, Sports, Science and Technology ; Japan Society for the Promotion of Science in Japan ; Japan Society for the Promotion of Science in Japan ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Institute for Cosmic Ray Research (ICRR) ; Institute for Cosmic Ray Research (ICRR) ; University of Tokyo ; University of Tokyo ; Ministry of Science and Technology of China ; Ministry of Science and Technology of China ; Ministry of Foreign Affairs of Japan ; Ministry of Foreign Affairs of Japan ; Ministry of Education, Culture, Sports, Science and Technology ; Ministry of Education, Culture, Sports, Science and Technology ; Japan Society for the Promotion of Science in Japan ; Japan Society for the Promotion of Science in Japan ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Institute for Cosmic Ray Research (ICRR) ; Institute for Cosmic Ray Research (ICRR) ; University of Tokyo ; University of Tokyo ; Ministry of Science and Technology of China ; Ministry of Science and Technology of China ; Ministry of Foreign Affairs of Japan ; Ministry of Foreign Affairs of Japan ; Ministry of Education, Culture, Sports, Science and Technology ; Ministry of Education, Culture, Sports, Science and Technology ; Japan Society for the Promotion of Science in Japan ; Japan Society for the Promotion of Science in Japan ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, CAS ; Institute for Cosmic Ray Research (ICRR) ; Institute for Cosmic Ray Research (ICRR) ; University of Tokyo ; University of Tokyo
WOS Research AreaPhysics
WOS SubjectPhysics, Multidisciplinary
WOS IDWOS:000674614700004
PublisherAMER PHYSICAL SOC
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/76582
Collection中国科学院国家天文台
Corresponding AuthorChen, D.; Huang, J.; Sako, T.; Takita, M.
Affiliation1.Hirosaki Univ, Dept Phys, Hirosaki, Aomori 0368561, Japan
2.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Peoples R China
3.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China
4.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
5.Tibet Univ, Dept Math & Phys, Lhasa 850000, Peoples R China
6.Hebei Normal Univ, Dept Phys, Shijiazhuang 050016, Hebei, Peoples R China
7.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
8.Shandong Univ, Inst Frontier & Interdisciplinary Sci, Qingdao 266237, Peoples R China
9.Shandong Univ, Key Lab Particle Phys & Particle Irradiat MOE, Qingdao 266237, Peoples R China
10.SouthWest Jiaotong Univ, Inst Modern Phys, Chengdu 610031, Peoples R China
11.Yokohama Natl Univ, Fac Engn, Yokohama, Kanagawa 2408501, Japan
12.Kanagawa Univ, Fac Engn, Yokohama, Kanagawa 2218686, Japan
13.Utsunomiya Univ, Fac Educ, Utsunomiya, Tochigi 3218505, Japan
14.Fac Syst Engn, Shibaura Inst Technol, Omiya, Saitama 3308570, Japan
15.Shinshu Univ, Dept Phys, Matsumoto, Nagano 3908621, Japan
16.Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan
17.Japan Aerosp Explorat Agcy ISAS JAXA, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2525210, Japan
18.China Meteorol Adm, Natl Ctr Space Weather, Beijing 100081, Peoples R China
19.Shandong Agr Univ, Sch Informat Sci & Engn, Tai An 271018, Shandong, Peoples R China
20.Univ Sci & Technol China, Sch Phys Sci, Dept Astron, Hefei 230026, Anhui, Peoples R China
21.Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China
22.Tsinghua Univ, Tsinghua Ctr Astrophys THCA, Beijing 100084, Peoples R China
23.Tsinghua Univ, Tsinghua Univ Natl Astron Observ China NAOC Joint, Beijing 100084, Peoples R China
24.Tsinghua Univ, Dept Astron, Beijing 100084, Peoples R China
25.Nihon Univ, Coll Ind Technol, Narashino, Chiba 2758575, Japan
26.Natl Inst Informat, Tokyo 1018430, Japan
27.Natl Inst Informat & Commun Technol, Tokyo 1848795, Japan
28.Shangdong Management Univ, Dept Mech & Elect Engn, Jinan 250357, Peoples R China
29.China Univ Petr, Coll Sci, Qingdao 266555, Shandong, Peoples R China
30.Tokyo Metropolitan Coll Ind Technol, Tokyo 1168523, Japan
31.Konan Univ, Dept Phys, Kobe, Hyogo 6588501, Japan
32.Shonan Inst Technol, Fujisawa, Kanagawa 2518511, Japan
33.Waseda Univ, Res Inst Sci & Engn, Tokyo 1620044, Japan
34.Japan Atom Energy Agcy, Tokai, Ibaraki 3191195, Japan
35.Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210034, Peoples R China
Recommended Citation
GB/T 7714
Amenomori, M.,Bao, Y. W.,Bi, X. J.,et al. Gamma-Ray Observation of the Cygnus Region in the 100-TeV Energy Region[J]. PHYSICAL REVIEW LETTERS,2021,127(3):6.
APA Amenomori, M..,Bao, Y. W..,Bi, X. J..,Chen, D..,Chen, T. L..,...&Zhou, X. X..(2021).Gamma-Ray Observation of the Cygnus Region in the 100-TeV Energy Region.PHYSICAL REVIEW LETTERS,127(3),6.
MLA Amenomori, M.,et al."Gamma-Ray Observation of the Cygnus Region in the 100-TeV Energy Region".PHYSICAL REVIEW LETTERS 127.3(2021):6.
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