REVERSE-SHOCK IN TYCHO'S SUPERNOVA REMNANT
文献类型：期刊论文
| 作者 | Lu FJ(卢方军) ; Ge MY(葛明玉); Zheng SJ(郑世界); Zhang SN(张双南); Long X(龙曦); Lu, FJ; Ge, MY; Zheng, SJ; Zhang, SN; Long, X
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| 刊名 | ASTROPHYSICAL JOURNAL
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| 出版日期 | 2015 |
| 卷号 | 805期号:2页码:142 |
| 关键词 | ISM: supernova remnants supernovae: general supernovae: individual (Tycho's SN) |
| 通讯作者 | 卢方军 |
| 英文摘要 | Thermal X-ray emission from young supernova remnants (SNRs) is usually dominated by the emission lines of the supernova ejecta, which are widely believed to be crossed and thus heated by the inward-propagating reverse shock (RS). Previous works using X-ray imaging data have shown that the ejecta are heated by the RS by locating the peak emission region of the most recently ionized matter, which is found to be well separated toward the inside from the outermost boundary. Here we report the discovery of a systematic increase of the Sulfur (S) to Silicon (Si) Ka line flux ratio with radius in Tycho's SNR. This allows us, for the first time, to present continuous radial profiles of the ionization age and, furthermore, the elapsed ionization time since the onset of the ionization, which gives the history of the propagation of the ionization front into the SNR ejecta. |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Astronomy & Astrophysics |
| 收录类别 | SCI ; CA |
| WOS记录号 | WOS:000356715400057 |
| 公开日期 | 2016-05-03 |
| 源URL | [http://ir.ihep.ac.cn/handle/311005/228404]  |
| 专题 | 高能物理研究所_粒子天体物理中心 |
| 推荐引用方式 GB/T 7714 | Lu FJ,Ge MY,Zheng SJ,et al. REVERSE-SHOCK IN TYCHO'S SUPERNOVA REMNANT[J]. ASTROPHYSICAL JOURNAL,2015,805(2):142. |
| APA | 卢方军.,葛明玉.,郑世界.,张双南.,龙曦.,...&Aschenbach, B.(2015).REVERSE-SHOCK IN TYCHO'S SUPERNOVA REMNANT.ASTROPHYSICAL JOURNAL,805(2),142. |
| MLA | 卢方军,et al."REVERSE-SHOCK IN TYCHO'S SUPERNOVA REMNANT".ASTROPHYSICAL JOURNAL 805.2(2015):142. |
入库方式： OAI收割
来源：高能物理研究所
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