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An ultrahigh-energy y-ray bubble powered by a super PeVatron
Cao, Z.1,2,3; Aharonian, F.4,5; An, Q.6,7; Axikegu8,9; Bai, Y. X.1,3; Bao, Y. W.10; Bastieri, D.11; Bi, X. J.1,2,3; Bi, Y. J.1,3; Cai, J. T.11; Cao, Q.12; Cao, W. Y.7; Cao, Zhe6,7; Chang, J.13,14; Chang, J. F.1,3,6; Chen, A. M.15,16; Chen, E. S.1,2,3; Chen, Liang17; Chen, Lin8,9; Chen, Long8,9; Chen, M. J.1,3; Chen, M. L.1,3,6; Chen, Q. H.8,9; Chen, S. H.1,2,3; Chen, S. Z.1,3; Chen, T. L.18; Chen, Y.10; Cheng, N.1,3; Cheng, Y. D.1,3; Cui, M. Y.13,14; Cui, S. W.12; Cui, X. H.19; Cui, Y. D.20,21,22; Dai, B. Z.23; Dai, H. L.1,3,6; Dai, Z. G.7; Danzengluobu18; della Volpe, D.24; Dong, X. Q.1,2,3; Duan, K. K.13,14; Fan, J. H.11; Fan, Y. Z.13,14; Fang, J.23; Fang, K.1,3; Feng, C. F.25; Feng, L.13,14; Feng, S. H.15,16; Feng, X. T.25; Feng, Y. L.18; Gabici, S.26; Gao, B.1,3; Gao, C. D.25; Gao, L. Q.1,2,3; Gao, Q.18; Gao, W.1,3; Gao, W. K.1,2,3; Ge, M. M.23; Geng, L. S.1,3; Giacinti, G.15,16; Gong, G. H.27; Gou, Q. B.1,3; Gu, M. H.1,3,6; Guo, F. L.17; Guo, X. L.8,9; Guo, Y. Q.1,3; Guo, Y. Y.13,14; Han, Y. A.28; He, H. H.1,2,3; He, H. N.13,14; He, J. Y.13,14; He, X. B.20,21,22; He, Y.8,9; Heller, M.24; Hor, Y. K.20,21,22; Hou, B. W.1,2,3; Hou, C.1,3; Hou X(侯贤)29; Hu, H. B.1,2,3; Hu, Q.7,13,14; Hu, S. C.1,2,3; Huang, D. H.8,9; Huang, T. Q.1,3; Huang, W. J.20,21,22; Huang, X. T.25; Huang, X. Y.13,14; Huang, Y.1,2,3; Huang, Z. C.8,9; Ji, X. L.1,3,6; Jia, H. Y.8,9; Jia, K.25; Jiang, K.6,7; Jiang, X. W.1,3; Jiang, Z. J.23; Jin, M.8,9; Kang, M. M.30; Ke, T.1,3; Kuleshov, D.31; Kurinov, K.31,32; Li, B. B.12; Li, Cheng6,7; Li, Cong1,3; Li, D.1,2,3; Li, F.1,3,6; Li, H. B.1,3; Li, H. C.1,3; Li, H. Y.7,13,14; Li, J.7,13,14; Li, Jian7; Li, Jie1,3,6; Li, K.1,3; Li, W. L.15,16,25; Li, X. R.1,3; Li, Xin6,7; Li, Y. Z.1,2,3; Li, Zhe1,3; Li, Zhuo33; Liang, E. W.34; Liang, Y. F.34; Lin, S. J.20,21,22; Liu, B.7; Liu, C.1,3; Liu, D.25; Liu, H.8,9; Liu, H. D.28; Liu, J.1,3; Liu, J. L.1,3; Liu, J. Y.1,3; Liu, M. Y.18; Liu, R. Y.10; Liu, S. M.8,9; Liu, W.1,3; Liu, Y.11; Liu, Y. N.27; Lu, R.23; Luo, Q.20,21,22; Lv, H. K.1,3; Ma, B. Q.33; Ma, L. L.1,3; Ma, X. H.1,3; Mao JR(毛基荣)29; Min, Z.1,3; Mitthumsiri, W.35; Mu, H. J.28; Nan, Y. C.1,3; Neronov, A.3,26; Ou, Z. W.20,21,22; Pang, B. Y.8,9; Pattarakijwanich, P.35; Pei, Z. Y.11; Qi, M. Y.1,3; Qi, Y. Q.12; Qiao, B. Q.1,3; Qin, J. J.7; Ruffolo, D.35; Saiz, A.3,35; Semikoz, D.26; Shao, C. Y.20,21,22; Shao, L.12; Shchegolev, O.31,32; Sheng, X. D.1,3; Shu, F. W.36,37,38; Song, H. C.33; Stenkin, Yu. V.31,32; Stepanov, V.31; Su, Y.13,14; Sun, Q. N.8,9; Sun, X. N.34; Sun, Z. B.39; Tam, P. H. T.20,21,22; Tang, Q. W.36,37,38; Tang, Z. B.6,7; Tian, W. W.2,19; Wang, C.39; Wang, C. B.8,9; Wang, G. W.7; Wang, H. G.11; Wang, H. H.20,21,22; Wang JC(王建成)29; Wang, K.10; Wang, L. P.25; Wang, L. Y.1,3; Wang, P. H.8,9; Wang, R.25; Wang, W.20,21,22; Wang, X. G.34; Wang, X. Y.10; Wang, Y.8,9; Wang, Y. D.1,3; Wang, Y. J.1,3; Wang, Z. H.; Wang, Z. X.23; Wang, Zhen15,16; Wang, Zheng1,3,6; Wei, D. M.13,14; Wei, J. J.13,14; Wei, Y. J.1,2,3; Wen, T.23; Wu, C. Y.1,3; Wu, H. R.1,3; Wu, S.1,3; Wu, X. F.13,14; Wu, Y. S.7; Xi, S. Q.1,3; Xia, J.7,13,14; Xia, J. J.8,9; Xiang, G. M.2,17; Xiao, D. X.12; Xiao, G.1,3; Xin, G. G.1,3; Xin, Y. L.8,9; Xing, Y.17; Xiong, Z.1,2,3; Xu, D. L.15,16; Xu, R. F.1,2,3; Xu, R. X.33; Xu, W. L.30; Xue, L.25; Yan, D. H.23; Yan, J. Z.13,14; Yan, T.1,3; Yang, C. W.30; Yang, F.12; Yang, F. F.1,3,6; Yang, H. W.20,21,22; Yang, J. Y.20,21,22; Yang, L. L.20,21,22; Yang, M. J.1,3; Yang, R. Z.7; Yang, S. B.23; Yao, Y. H.30; Yao, Z. G.1,3; Ye, Y. M.27; Yin, L. Q.1,3; Yin, N.25; You, X. H.1,3; You, Z. Y.1,2,3; Yu, Y. H.7; Yuan, Q.13,14; Yue, H.1,2,3; Zeng, H. D.13,14; Zeng, T. X.1,3,6; Zeng, W.23; Zha, M.1,3; Zhang, B. B.10; Zhang, F.8,9; Zhang, H. M.10; Zhang, H. Y.1,3; Zhang, J. L.19; Zhang, L. X.11; Zhang, Li23; Zhang, P. F.23; Zhang, P. P.7,13,14; Zhang, R.7,13,14; Zhang, S. B.2,19; Zhang, S. R.12; Zhang, S. S.1,3; Zhang, X.10; Zhang, X. P.1,3; Zhang, Y. F.8,9; Zhang, Yi1,13,14; Zhang, Yong1,3; Zhao, B.8,9; Zhao, J.1,3; Zhao, L.6,7; Zhao, L. Z.12; Zhao, S. P.13,14,25; Zheng, F.39; Zhou, B.1,3; Zhou, H.15,16; Zhou, J. N.17; Zhou, M.36,37,38; Zhou, P.10; Zhou, R.30; Zhou, X. X.8,9; Zhu, C. G.25; Zhu, F. R.8,9; Zhu, H.19; Zhu, K. J.1,2,3,6; Zuo, X.1,3
发表期刊SCIENCE BULLETIN
2024-02-26
卷号69期号:4页码:449-457
DOI10.1016/j.scib.2023.12.040
产权排序第29完成单位
收录类别SCI
关键词Cosmic rays y-rays Interstellar medium Star cluster
摘要We report the detection of a y-ray bubble spanning at least 100 deg2 in ultra-high energy (UHE) up to a few PeV in the direction of the star-forming region Cygnus X, implying the presence super PeVatron(s) accelerating protons to at least 10 PeV. A log-parabola form with the photon index C(E) = (2.71 +/- 0.02) + (0.11 +/- 0.02) x log10(E/10 TeV) is found fitting the gamma-ray energy spectrum of the bubble well. UHE sources, hot spots correlated with very massive molecular clouds, and a quasi-spherical amorphous y-ray emitter with a sharp central brightening are observed in the bubble. In the core of - 0.5 degrees, spatially associating with a region containing massive OB association (Cygnus OB2) and a microquasar (Cygnus X-3), as well as previously reported multi-TeV sources, an enhanced concentration of UHE y-rays is observed with 2 photons at energies above 1 PeV. The general feature of the bubble, the morphology, and the energy spectrum, are reasonably reproduced by the assumption of a particle accelerator in the core, continuously injecting protons into the ambient medium. (c) 2023 Science China Press. Published by Elsevier B.V. and Science China Press. All rights reserved.
资助项目Chengdu Management Committee of Tianfu New Area
项目资助者Chengdu Management Committee of Tianfu New Area
语种英语
学科领域天文学
文章类型Article
出版者ELSEVIER
出版地RADARWEG 29, 1043 NX AMSTERDAM, NETHERLANDS
ISSN2095-9273
URL查看原文
WOS记录号WOS:001185327600001
WOS研究方向Science & Technology - Other Topics
WOS类目Multidisciplinary Sciences
引用统计
被引频次：32[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/26550
专题星系类星体研究组
高能天体物理研究组
作者单位1.Chinese Acad Sci, Key Lab Particle Astrophy & Expt Phys, Div & Comp Ctr, Inst High Energy Phys, Beijing 100049, Peoples R China;
2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China;
3.TIANFU Cosm Ray Res Ctr, Chengdu, Peoples R China;
4.Dublin Inst Adv Studies, 31 Fitzwilliam Pl, Dublin 2, Ireland;
5.Max Planck Inst Nucl Phys, POB 103980, D-69026 Heidelberg, Germany;
6.State Key Lab Particle Detect & Elect, Beijing, Peoples R China;
7.Univ Sci & Technol China, Hefei 230026, Peoples R China;
8.Southwest Jiaotong Univ, Sch Phys Sci & Technol, Chengdu 610031, Peoples R China;
9.Southwest Jiaotong Univ, Sch Informat Sci & Technol, Chengdu 610031, Peoples R China;
10.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Peoples R China;
11.Guangzhou Univ, Ctr Astrophys, Guangzhou 510006, Peoples R China;
12.Hebei Normal Univ, Shijiazhuang 050024, Peoples R China;
13.Chinese Acad Sci, Key Lab Dark Matter & Space Astron, Nanjing 210023, Peoples R China;
14.Chinese Acad Sci, Key Lab Radio Astron, Purple Mt Observ, Nanjing 210023, Peoples R China;
15.Shanghai Jiao Tong Univ, Tsung Dao Lee Inst, Shanghai 200240, Peoples R China;
16.Shanghai Jiao Tong Univ, Sch Phys & Astron, Shanghai 200240, Peoples R China;
17.Chinese Acad Sci, Key Lab Res Galaxies & Cosmol, Shanghai Astron Observ, Shanghai 200030, Peoples R China;
18.Tibet Univ, Key Lab Cosm Rays, Minist Educ, Lhasa 850000, Peoples R China;
19.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China;
20.Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai 519000, Peoples R China;
21.Sun Yat Sen Univ, Sch Phys, Guangzhou 510275, Peoples R China;
22.Sun Yat Sen Univ, Sino French Inst Nucl Engn & Technol, Zhuhai 519000, Peoples R China;
23.Yunnan Univ, School Phys & Astron, Kunming 650091, Peoples R China;
24.Univ Geneva, Dept Phys Nucl & Corpusculaire, Fac Sci, 24 Quai Ernest Ansermet, CH-1211 Geneva, Switzerland;
25.Shandong Univ, Inst Frontier & Interdisciplinary Sci, Qingdao 266237, Peoples R China;
26.Univ Paris Cite, CNRS, IN2P3, CEA,IRFU,Observ Paris, F-75205 Paris, France;
27.Tsinghua Univ, Dept Engn Phys, Beijing 100084, Peoples R China;
28.Zhengzhou Univ, Sch Phys & Microelect, Zhengzhou 450001, Peoples R China;
29.Chinese Acad Sci, Yunnan Observ, Kunming 650216, Peoples R China;
30.Sichuan Univ, Coll Phys, Chengdu 610065, Sichuan, Peoples R China;
31.Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia;
32.Moscow Inst Phys & Technol, Moscow 141700, Russia;
33.Peking Univ, Sch Phys, Beijing 100871, Peoples R China;
34.Guangxi Univ, Sch Phys Sci & Technol, Nanning 530004, Peoples R China;
35.Mahidol Univ, Dept Phys, Fac Sci, Bangkok 10400, Thailand;
36.Nanchang Univ, Ctr Relativist Astrophys & High Energy Phys, Nanchang 330031, Peoples R China;
37.Nanchang Univ, Sch Phys & Mat Sci, Nanchang 330031, Peoples R China;
38.Nanchang Univ, Inst Space Sci & Technol, Nanchang 330031, Peoples R China;
39.Chinese Acad Sci, Natl Space Sci Ctr, Beijing 100190, Peoples R China
推荐引用方式
GB/T 7714		 Cao, Z.,Aharonian, F.,An, Q.,et al. An ultrahigh-energy y-ray bubble powered by a super PeVatron[J]. SCIENCE BULLETIN,2024,69(4):449-457.
APA Cao, Z..,Aharonian, F..,An, Q..,Axikegu.,Bai, Y. X..,...&Zuo, X..(2024).An ultrahigh-energy y-ray bubble powered by a super PeVatron.SCIENCE BULLETIN,69(4),449-457.
MLA Cao, Z.,et al."An ultrahigh-energy y-ray bubble powered by a super PeVatron".SCIENCE BULLETIN 69.4(2024):449-457.
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