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题名: The structure of TeV-bright shell-type supernova remnants
作者: Yang, Chuyuan1, 2; Liu SiMing(刘四明)3; Fang, Jun4; Li Hui(黎辉)5
刊名: ASTRONOMY & ASTROPHYSICS
出版日期: 2015
卷号: 573, 页码:A37
关键词: turbulence ; shock waves ; radiation mechanisms: non-thermal
学科分类: 天文和天体物理
DOI: 10.1051/0004-6361/201424667
文章类型: Article
英文摘要: Aims. Two-dimensional magnetohydrodynamic (MHD) simulations are used to model the emission properties of TeV-bright shell-type supernova remnants (SNRs) and to explore their nature.
WOS标题词: Science & Technology ; Physical Sciences
类目[WOS]: Astronomy & Astrophysics
研究领域[WOS]: Astronomy & Astrophysics
关键词[WOS]: SNR RX J1713.7-3946 ; GAMMA-RAY EMISSION ; LARGE-AREA TELESCOPE ; STOCHASTIC ELECTRON ACCELERATION ; MAGNETIC-FIELD AMPLIFICATION ; RCW 86 ; COSMIC-RAYS ; HESS J1731-347 ; SYNCHROTRON EMISSION ; SHOCK-WAVE
收录类别: SCI
所属项目名称: PMO_LIB-IR
语种: 英语
WOS记录号: WOS:000346901300065
Citation statistics:
内容类型: 期刊论文
URI标识: http://libir.pmo.ac.cn/handle/332002/14833
Appears in Collections:太阳高能及相关物理过程研究团组_期刊论文

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作者单位: 1.Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China
2.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650011, Peoples R China
3.Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210008, Jiangsu, Peoples R China
4.Yunnan Univ, Dept Astron, Kunming 650091, Peoples R China
5.Los Alamos Natl Lab, Los Alamos, NM 87545 USA
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