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Observation of the γ-ray emission from W43 with LHAASO
Cao, Zhen1,2,3; Aharonian, F.4,5; Axikegu6; Bai, Y. X.1,3; Bao, Y. W.7; Bastieri, D.8; Bi, X. J.1,2,3; Bi, Y. J.1,3; Bian, W.9; Bukevich, A. V.10; Cao, Q.11; Cao, W. Y.12; Cao, Zhe12,13; Chang, J.14; Chang, J. F.1,3,13; Chen, A. M.9; Chen, E. S.1,2,3; Chen, H. X.15; Chen, Liang16; Chen, Lin6; Chen, Long6; Chen, M. J.1,3; Chen, M. L.1,3,13; Chen, Q. H.6; Chen, S.17; Chen, S. H.1,2,3; Chen, S. Z.1,3; Chen, T. L.18; Chen, Y.7; Cheng, N.1,3; Cheng, Y. D.1,2,3; Chu, M. C.19; Cui, M. Y.14; Cui, S. W.11; Cui, X. H.20; Cui, Y. D.21,22; Dai, B. Z.17; Dai, H. L.1,3,13; Dai, Z. G.12; Danzengluobu18; Dong, X. Q.1,2,3; Duan, K. K.14; Fan, J. H.8; Fan, Y. Z.14; Fang, J.17; Fang, J. H.15; Fang, K.13; Feng, C. F.23; Feng, H.1; Feng, L.14; Feng, S. H.1,3; Feng, X. T.23; Feng, Y.15; Feng, Y. L.18; Gabici, S.24; Gao, B.1,3; Gao, C. D.23; Gao, Q.18; Gao, W.1,3; Gao, W. K.1,2,3; Ge, M. M.17; Ge, T. T.21,22; Geng, L. S.1,3; Giacinti, G.9; Gong, G. H.25; Gou, Q. B.1,3; Gu, M. H.1,3,13; Guo, F. L.16; Guo, J.25; Guo, X. L.6; Guo, Y. Q.1,3; Guo, Y. Y.14; Han, Y. A.26; Hannuksela, O. A.19; Hasan, M.1,2,3; He, H. H.1,2,3; He, H. N.14; He, J. Y.14; He, Y.6; Hor, Y. K.21,22; Hou, B. W.1,2,3; Hou, C.1,3; Hou X(侯贤)27; Hu, H. B.1,2,3; Hu, Q.12,14; Hu, S. C.1,3,28; Huang, C.7; Huang, D. H.6; Huang, T. Q.1,3; Huang, W. J.21,22; Huang, X. T.23; Huang, X. Y.14; Huang, Y.1,2,3; Huang, Y. Y.7; Ji, X. L.1,3,13; Jia, H. Y.6; Jia, K.23; Jiang, H. B.1,3; Jiang, K.12,13; Jiang, X. W.1,3; Jiang, Z. J.17; Jin, M.6; Kang, M. M.29; Karpikov, I.10; Khangulyan, D.1,3; Kuleshov, D.10; Kurinov, K.10; Li, B. B.11; Li, C. M.7; Li, Cheng12,13; Li, Cong1,3; Li, D.1,2,3; Li, F.1,3,13; Li, H. B.1,3; Li, H. C.1,3; Li, Jian12; Li, Jie1,3,13; Li, K.1,3; Li, S. D.2,16; Li, W. L.23; Li, W. L.9; Li, X. R.1,3; Li, Xin12,13; Li, Y. Z.1,2,3; Li, Zhe1,3; Li, Zhuo30; Liang, E. W.31; Liang, Y. F.31; Lin, S. J.21,22; Liu, B.12; Liu, C.1,3; Liu, D.23; Liu, D. B.9; Liu, H.6; Liu, H. D.26; Liu, J.1,3; Liu, J. L.1,3; Liu, M. Y.18; Liu, R. Y.7; Liu, S. M.6; Liu, W.1,3; Liu, Y.8; Liu, Y. N.25; Luo, Q.21,22; Luo, Y.9; Lv, H. K.1,3; Ma, B. Q.30; Ma, L. L.1,3; Ma, X. H.1,3; Mao JR(毛基荣)27; Min, Z.1,3; Mitthumsiri, W.32; Mu, H. J.26; Nan, Y. C.1,3; Neronov, A.24; Ng, K. C. Y.19; Ou, L. J.8; Pattarakijwanich, P.32; Pei, Z. Y.8; Qi, J. C.1,2,3; Qi, M. Y.1,3; Qiao, B. Q.1,3; Qin, J. J.12; Raza, A.1,2,3; Ruffolo, D.32; Sáiz, A.32; Saeed, M.1,2,3; Semikoz, D.24; Shao, L.11; Shchegolev, O.10,33; Sheng, X. D.1,3; Shu, F. W.34; Song, H. C.30; Stenkin, Yu. V.10,33; Stepanov, V.10; Su, Y.14; Sun, D. X.12,14; Sun, Q. N.6; Sun, X. N.31; Sun, Z. B.35; Takata, J.36; Tam, P. H. T.21,22; Tang, Q. W.34; Tang, R.9; Tang, Z. B.12,13; Tian, W. W.2,20; Wan, L. H.21,22; Wang, C.35; Wang, C. B.6; Wang, G. W.12; Wang, H. G.8; Wang, H. H.21,22; Wang JC(王建成)27; Wang, Kai7; Wang, Kai36; Wang, L. P.1,2,3; Wang, L. Y.1,3; Wang, P. H.6; Wang, R.23; Wang, W.21,22; Wang, X. G.31; Wang, X. Y.7; Wang, Y.6; Wang, Y. D.1,3; Wang, Y. J.1,3; Wang, Z. H.29; Wang, Z. X.17; Wang, Zhen9; Wang, Zheng1,3,13; Wei, D. M.14; Wei, J. J.14; Wei, Y. J.1,2,3; Wen, T.17; Wu, C. Y.1,3; Wu, H. R.1,3; Wu, Q. W.36; Wu, S.1,3; Wu, X. F.14; Wu, Y. S.12; Xi, S. Q.1,3; Xia, J.12,14; Xiang, G. M.2,16; Xiao, D. X.11; Xiao, G.1,3; Xin, Y. L.6; Xing, Y.16; Xiong DR(熊定荣)27; Xiong, Z.1,2,3; Xu, D. L.9; Xu, R. F.1,2,3; Xu, R. X.30; Xu, W. L.29; Xue, L.23; Yan, D. H.17; Yan, J. Z.14; Yan, T.1,3; Yang, C. W.29; Yang CY(杨初源)27; Yang, F.11; Yang, F. F.1,3,13; Yang, L. L.21,22; Yang, M. J.1,3; Yang, R. Z.3,12; Yang, W. X.8; Yao, Y. H.1,3; Yao, Z. G.1,3; Yin, L. Q.1,3; Yin, N.23; You, X. H.1,3; You, Z. Y.1,3; Yu, Y. H.12; Yuan, Q.14; Yue, H.1,2,3; Zeng, H. D.14; Zeng, T. X.1,3,13; Zeng, W.17; Zha, M.1,3; Zhang, B. B.7; Zhang, F.6; Zhang, H.9; Zhang, H. M.7; Zhang, H. Y.17; Zhang, J. L.20; Zhang, Li17; Zhang, P. F.17; Zhang, P. P.12,14; Zhang, R.14; Zhang, S. B.2,20; Zhang, S. R.11; Zhang, S. S.1,3; Zhang, X.7; Zhang, X. P.1,3; Zhang, Y. F.6; Zhang, Yi1,14; Zhang, Yong1,3; Zhao, B.6; Zhao, J.1,3; Zhao, L.12,13; Zhao, L. Z.11; Zhao, S. P.14; Zhao XH(赵晓红)27; Zheng, F.35; Zhong, W. J.7; Zhou, B.1,3; Zhou, H.9; Zhou, J. N.16; Zhou, M.34; Zhou, P.7; Zhou, R.29; Zhou, X. X.1,2,3; Zhou, X. X.6; Zhu, B. Y.12,14; Zhu, C. G.23; Zhu, F. R.6; Zhu, H.20; Zhu, K. J.1,2,3,13; Zou, Y. C.36; Zuo, X.1,3
发表期刊SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
2024-07
卷号68期号:7
DOI10.1007/s11433-024-2477-9
产权排序第27完成单位
收录类别SCI ; EI
关键词gamma-ray source cosmic rays star formation region
摘要In this paper, we report the detection of the very-high-energy (VHE, 100 GeV < E < 100 TeV) and ultra-high-energy (UHE, E > 100 TeV) gamma-ray emissions from the direction of the young star-forming region W43, observed by the Large High Altitude Air Shower Observation (LHAASO). The extended gamma-ray source was detected with a significance of similar to 16 sigma by KM2A and similar to 17 sigma by WCDA, respectively. The angular extension of this gamma-ray source is about 0.5 degrees, corresponding to a physical size of about 50 pc. We discuss the origin of the gamma-ray emission and possible cosmic ray acceleration in the W43 region using multi-wavelength data. Our findings suggest that W43 is likely another young star cluster capable of accelerating cosmic rays (CRs) to at least several hundred TeV.
资助项目Chengdu Management Committee of Tianfu New Area; National Natural Science Foundation of China[12393854]; National Natural Science Foundation of China[12175121]; National Natural Science Foundation of China[12393851]; National Natural Science Foundation of China[12393852]; National Natural Science Foundation of China[12393853]; National Natural Science Foundation of China[12205314]; National Natural Science Foundation of China[12105301]; National Natural Science Foundation of China[12305120]; National Natural Science Foundation of China[12261160362]; National Natural Science Foundation of China[12105294]; National Natural Science Foundation of China[U1931201]; National Natural Science Foundation of China[12375107]; National Natural Science Foundation of China[12173039]; Department of Science and Technology of Sichuan Province, China[24NSFSC2319]; Project for Young Scientists in Basic Research of Chinese Academy of Sciences[YSBR-061]; National Science and Technology Development Agency (NSTDA); National Research Council of Thailand (NRCT) under the High-Potential Research Team Grant Program[N42A650868]
项目资助者Chengdu Management Committee of Tianfu New Area ; National Natural Science Foundation of China[12393854, 12175121, 12393851, 12393852, 12393853, 12205314, 12105301, 12305120, 12261160362, 12105294, U1931201, 12375107, 12173039] ; Department of Science and Technology of Sichuan Province, China[24NSFSC2319] ; Project for Young Scientists in Basic Research of Chinese Academy of Sciences[YSBR-061] ; National Science and Technology Development Agency (NSTDA) ; National Research Council of Thailand (NRCT) under the High-Potential Research Team Grant Program[N42A650868]
语种英语
学科领域天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学
文章类型Article
出版者SCIENCE PRESS
出版地16 DONGHUANGCHENGGEN NORTH ST, BEIJING 100717, PEOPLES R CHINA
ISSN1674-7348
URL查看原文
WOS记录号WOS:001413219500001
WOS研究方向Physics
WOS类目Physics, Multidisciplinary
关键词[WOS]CRAB-NEBULA ; TRANSPORT ; PULSARS ; COMPLEX ; MODEL
引用统计
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/28167
专题星系类星体研究组
高能天体物理研究组
南方基地
作者单位1.Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China;
2.University of Chinese Academy of Sciences, Beijing, 100049, China;
3.TIANFU Cosmic Ray Research Center, Chengdu, China;
4.Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2, Dublin, Ireland;
5.Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg, 69029, Germany;
6.School of Physical Science and Technology & School of Information Science and Technology, Southwest Jiaotong University, Chengdu, 610031, China;
7.School of Astronomy and Space Science, Nanjing University, Nanjing, 210023, China;
8.Center for Astrophysics, Guangzhou University, Guangzhou, 510006, China;
9.Tsung-Dao Lee Institute & School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China;
10.Institute for Nuclear Research of Russian Academy of Sciences, Moscow, 117312, Russia;
11.Hebei Normal University, Shijiazhuang, 050024, China;
12.University of Science and Technology of China, Hefei, 230026, China;
13.State Key Laboratory of Particle Detection and Electronics, Beijing, China;
14.Key Laboratory of Dark Matter and Space Astronomy & Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210023, China;
15.Research Center for Astronomical Computing, Zhejiang Laboratory, Hangzhou, 311121, China;
16.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China;
17.School of Physics and Astronomy, Yunnan University, Kunming, 650091, China;
18.Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Lhasa, 850000, China;
19.Department of Physics, The Chinese University of Hong Kong, Shatin, New Territories, Hong Kong, 999077, China;
20.Key Laboratory of Radio Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China;
21.School of Physics and Astronomy (Zhuhai) & Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Zhuhai, 519000, China;
22.School of Physics (Guangzhou), Sun Yat-sen University, Guangzhou, 510275, China;
23.Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao, 266237, China;
24.APC, Université Paris Cité, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, Paris 119, 75205, France;
25.Department of Engineering Physics & Department of Astronomy, Tsinghua University, Beijing, 100084, China;
26.School of Physics and Microelectronics, Zhengzhou University, Zhengzhou, 450001, China;
27.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, China;
28.China Center of Advanced Science and Technology, Beijing, 100190, China;
29.College of Physics, Sichuan University, Chengdu, 610065, China;
30.School of Physics, Peking University, Beijing, 100871, China;
31.Guangxi Key Laboratory for Relativistic Astrophysics, School of Physical Science and Technology, Guangxi University, Nanning, 530004, China;
32.Department of Physics, Faculty of Science, Mahidol University, Bangkok, 10400, Thailand;
33.Moscow Institute of Physics and Technology, Moscow, 141700, Russia;
34.Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science & Institute of Space Science and Technology, Nanchang University, Nanchang, 330031, China;
35.National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China;
36.School of Physics, Huazhong University of Science and Technology, Wuhan, 430074, China
推荐引用方式
GB/T 7714		 Cao, Zhen,Aharonian, F.,Axikegu,et al. Observation of the γ-ray emission from W43 with LHAASO[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2024,68(7).
APA Cao, Zhen.,Aharonian, F..,Axikegu.,Bai, Y. X..,Bao, Y. W..,...&Zuo, X..(2024).Observation of the γ-ray emission from W43 with LHAASO.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,68(7).
MLA Cao, Zhen,et al."Observation of the γ-ray emission from W43 with LHAASO".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 68.7(2024).
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