The single-degenerate binary origin of tycho's supernova as traced by the stripped envelope of the companion
文献类型：期刊论文
| 作者 | Lu, F. J.1; Wang, Q. D.2; Ge, M. Y.1; Qu, J. L.1; Yang, X. J.3; Zheng, S. J.1; Chen, Y.1 |
| 刊名 | Astrophysical journal
 |
| 出版日期 | 2011-05-01 |
| 卷号 | 732期号:1页码:6 |
| 关键词 | Ism: supernova remnants Supernovae: general Supernovae: individual (tycho's star) |
| ISSN号 | 0004-637X |
| DOI | 10.1088/0004-637x/732/1/11 |
| 通讯作者 | Lu, f. j.(lufj@mail.ihep.ac.cn) |
| 英文摘要 | We propose that a nonthermal x-ray arc inside the remnant of tycho's supernova (sn) represents the interaction between the sn ejecta and the companion star's envelope lost in the impact of the explosion. the x-ray emission of the remnant further shows an apparent shadow casted by the arc in the opposite direction of the explosion site, consistent with the blocking of the sn ejecta by the envelope. this scenario supports the single degenerate binary origin of tycho's sn. the properties of the x-ray arc, together with the previous detection of the companion candidate and its space velocity by ruiz-lapuente et al. and hernandez et al., enable us to further infer that (1) the progenitor binary has a period of 4.9(-3.0)(+5.3) days, (2) the companion gained a kick velocity of 42 +/- 30 km s(-1), and (3) the stripped envelope mass is about 0.0016 (<= 0.0083) m-circle dot. however, we note that the nature of the companion candidate is still under debate, and the above parameters need to be revised according to the actual properties of the companion candidate. further work to measure the proper motion of the arc and to check the capability of the interaction to emit the amount of x-rays observed from the arc is also needed to validate the current scenario. |
| WOS关键词 | REMNANT ; SYSTEMS ; IMPACT ; STAR ; PROGENITOR ; EXPLOSIONS ; EVOLUTION ; MODELS ; CLOUD ; SHOCK |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:000289626500011 |
| 出版者 | IOP PUBLISHING LTD |
| URI标识 | http://www.irgrid.ac.cn/handle/1471x/2176053 |
| 专题 | 高能物理研究所 |
| 通讯作者 | Lu, F. J. |
| 作者单位 | 1.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China 2.Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA 3.Xiangtan Univ, Fac Mat Optoelect & Phys, Xiangtan 411105, Hunan, Peoples R China |
| 推荐引用方式 GB/T 7714 | Lu, F. J.,Wang, Q. D.,Ge, M. Y.,et al. The single-degenerate binary origin of tycho's supernova as traced by the stripped envelope of the companion[J]. Astrophysical journal,2011,732(1):6. |
| APA | Lu, F. J..,Wang, Q. D..,Ge, M. Y..,Qu, J. L..,Yang, X. J..,...&Chen, Y..(2011).The single-degenerate binary origin of tycho's supernova as traced by the stripped envelope of the companion.Astrophysical journal,732(1),6. |
| MLA | Lu, F. J.,et al."The single-degenerate binary origin of tycho's supernova as traced by the stripped envelope of the companion".Astrophysical journal 732.1(2011):6. |
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