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Does or Did the Supernova Remnant Cassiopeia A Operate as a PeVatron?

文献类型：期刊论文

作者Cao,Zhen23,24,25; Aharonian,F.21,22; An,Q.19,20; Axikegu,18; Bai,Y. X.23,25; Bao,Y. W.17; Bastieri,D.16; Bi,X. J.23,24,25; Bi,Y. J.23,25; Cai,J. T.16
刊名The Astrophysical Journal Letters
出版日期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
WOS关键词COSMIC-RAY ACCELERATION ; MAGNETIC-FIELD ; SHOCK ACCELERATION ; TEV ENERGIES ; A SUPERNOVA ; SPECTRUM ; EMISSION ; OBLIQUE ; ESCAPE ; GAS
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]
源URL[http://ir.ynao.ac.cn/handle/114a53/26659]  
专题星系类星体研究组
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.Hebei Normal University, 050024 Shijiazhuang, Hebei, People's Republic of China
2.Institute for Nuclear Research of Russian Academy of Sciences, 117312 Moscow, Russia
3.Yunnan Observatories, Chinese Academy of Sciences, 650216 Kunming, Yunnan, People's Republic of China
4.School of Physics and Microelectronics, Zhengzhou University, 450001 Zhengzhou, Henan, People's Republic of China
5.Department of Engineering Physics, Tsinghua University, 100084 Beijing, People's Republic of China
6.APC, Université Paris Cité, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, 119, F-75205 Paris, France
7.Institute of Frontier and Interdisciplinary Science, Shandong University, 266237 Qingdao, Shandong, People's Republic of China
8.Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, 1211 Geneva, Switzerland
9.School of Physics and Astronomy, Yunnan University, 650091 Kunming, Yunnan, People's Republic of China
10.School of Physics and Astronomy (Zhuhai) & School of Physics (Guangzhou) & Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, 519000 Zhuhai & 510275 Guangzhou, Guangdong, 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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