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 |
DOI | 10.3847/2041-8213/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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