Does or Did the Supernova Remnant Cassiopeia A Operate as a PeVatron?
Cao,Zhen2,3,4; Aharonian,F.5,6; An,Q.7,8; Axikegu,9; Bai,Y. X.2,4; Bao,Y. W.10; Bastieri,D.11; Bi,X. J.2,3,4; Bi,Y. J.2,4; Cai,J. T.11
刊名The Astrophysical Journal Letters
2024-01-30
卷号961期号:2
ISSN号2041-8205
DOI10.3847/2041-8213/ad1d62
产权排序第24完成单位
文献子类Article
学科主题天文学
URL标识查看原文
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
资助项目National Key R&D program of China[2018YFA0404201]; National Key R&D program of China[2018YFA0404202]; National Key R&D program of China[2018YFA0404203]; National Key R&D program of China[2018YFA0404204]; National Natural Science Foundation of China NSFC[12022502]; National Natural Science Foundation of China NSFC[12205314]; National Natural Science Foundation of China NSFC[12105301]; National Natural Science Foundation of China NSFC[12261160362]; National Natural Science Foundation of China NSFC[12105294]; National Natural Science Foundation of China NSFC[U1931201]; National Science and Technology Development Agency (NSTDA); National Research Council of Thailand (NRCT) under the High-Potential Research Team grant program[N42A650868]
WOS关键词COSMIC-RAY ACCELERATION ; MAGNETIC-FIELD ; SHOCK ACCELERATION ; TEV ENERGIES ; A SUPERNOVA ; SPECTRUM ; EMISSION ; OBLIQUE ; ESCAPE ; GAS
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP Publishing Ltd
WOS记录号WOS:001187909900001
资助机构National Key R&D program of China[2018YFA0404201, 2018YFA0404202, 2018YFA0404203, 2018YFA0404204] ; National Natural Science Foundation of China NSFC[12022502, 12205314, 12105301, 12261160362, 12105294, U1931201] ; National Science and Technology Development Agency (NSTDA) ; National Research Council of Thailand (NRCT) under the High-Potential Research Team grant program[N42A650868]
内容类型期刊论文
源URL[http://ir.ynao.ac.cn/handle/114a53/26659]  
专题云南天文台_高能天体物理研究组
通讯作者Yang,R. Z.
作者单位1.National Space Science Center, Chinese Academy of Sciences, 100190 Beijing, People's Republic of China
2.Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, People's Republic of China;
3.University of Chinese Academy of Sciences, 100049 Beijing, People's Republic of China
4.Tianfu Cosmic Ray Research Center, 610000 Chengdu, Sichuan, People's Republic of China
5.Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland; felix.aharonian@mpi-hd.mpg.de
6.Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, D-69029 Heidelberg, Germany
7.State Key Laboratory of Particle Detection and Electronics, People's Republic of China
8.University of Science and Technology of China, 230026 Hefei, Anhui, People's Republic of China; yangrz@ustc.edu.cn
9.School of Physical Science and Technology & School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, People's Republic of China; yuyh@ustc.edu.cn
10.School of Astronomy and Space Science, Nanjing University, 210023 Nanjing, Jiangsu, People's Republic of China
推荐引用方式
GB/T 7714
Cao,Zhen,Aharonian,F.,An,Q.,et al. Does or Did the Supernova Remnant Cassiopeia A Operate as a PeVatron?[J]. The Astrophysical Journal Letters,2024,961(2).
APA Cao,Zhen.,Aharonian,F..,An,Q..,Axikegu,.,Bai,Y. X..,...&,.(2024).Does or Did the Supernova Remnant Cassiopeia A Operate as a PeVatron?.The Astrophysical Journal Letters,961(2).
MLA Cao,Zhen,et al."Does or Did the Supernova Remnant Cassiopeia A Operate as a PeVatron?".The Astrophysical Journal Letters 961.2(2024).
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