The structure of TeV-bright shell-type supernova remnants
文献类型：期刊论文
| 作者 | Yang, Chuyuan1,2; Liu, Siming3 ; Fang, Jun4; Li, Hui5
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| 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 |
| 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 |
| 学科主题 | 天文和天体物理 |
| 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 |
| 语种 | 英语 |
| WOS记录号 | WOS:000346901300065 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/14833]  |
| 专题 | 紫金山天文台_太阳高能及相关物理过程研究团组 |
| 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 |
| 推荐引用方式 GB/T 7714 | Yang, Chuyuan,Liu, Siming,Fang, Jun,et al. The structure of TeV-bright shell-type supernova remnants[J]. ASTRONOMY & ASTROPHYSICS,2015,573:A37. |
| APA | Yang, Chuyuan,Liu, Siming,Fang, Jun,&Li, Hui.(2015).The structure of TeV-bright shell-type supernova remnants.ASTRONOMY & ASTROPHYSICS,573,A37. |
| MLA | Yang, Chuyuan,et al."The structure of TeV-bright shell-type supernova remnants".ASTRONOMY & ASTROPHYSICS 573(2015):A37. |
入库方式： OAI收割
来源：紫金山天文台
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