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THE EXTREMELY LONG-PERIOD X-RAY SOURCE IN A YOUNG SUPERNOVA REMNANT: A THORNE-ZYTKOW OBJECT DESCENDANT?

文献类型：期刊论文

作者Liu, XW1,2; Xu, RX2; van den Heuvel, EPJ3; Qiao, GJ2; Han, JL4; Han ZW(韩占文)5; Li, XD6
刊名ASTROPHYSICAL JOURNAL
出版日期2015-02-01
卷号799期号:2
关键词ISM: supernova remnants stars: evolution stars: individual (1E161348-5055) stars: neutron
ISSN号0004-637X
产权排序第五完成单位
通讯作者Liu, XW (reprint author), China West Normal Univ, Sch Phys & Elect Informat, Nanchong 637002, Peoples R China.
英文摘要The origin of the 6.67 hr period X-ray source, 1E161348-5055, in the young supernova remnant RCW 103 is puzzling. We propose that it may be the descendant of a Thorne-Zytkow Object (TZO). A TZO may at its formation have a rapidly spinning neutron star as a core and a slowly rotating envelope. We found that the core could be braked quickly to an extremely long spin period by the coupling between its magnetic field and the envelope, and that the envelope could be disrupted by some powerful bursts or exhausted via stellar wind. If the envelope is disrupted after the core has spun down, the core will become an extremely long-period compact object, with a slow proper motion speed, surrounded by a supernova-remnant-like shell. These features all agree with the observations of 1E161348-5055. TZOs are expected to have produced extraordinarily high abundances of lithium and rapid proton process elements that would remain in the remnants and could be used to test this scenario.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]ACTIVE GALACTIC NUCLEI ; BLACK-HOLES ; GALAXIES ; FEEDBACK ; LINE ; MOTIONS ; MERGERS ; MASSES
收录类别SCI
原文出处http://iopscience.iop.org/article/10.1088/0004-637X/799/2/233/meta
语种英语
WOS记录号WOS:000348820900120
源URL[http://ir.ynao.ac.cn/handle/114a53/4604]  
专题云南天文台_大样本恒星演化研究组
云南天文台_中国科学院天体结构与演化重点实验室
作者单位1.School of Physics and Electronic Information, China West Normal University, Nanchong 637002, China
2.School of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China
3.Astronomical Institute Anton Pannekoek, University of Amsterdam, The Netherlands
4.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
5.Key Laboratory of the Structure and Evolution of Celestial Objects, Yunnan Observatory, Kunming 650011, China
6.Department of Astronomy, Nanjing University, Nanjing 210093, China
推荐引用方式
GB/T 7714		 Liu, XW,Xu, RX,van den Heuvel, EPJ,et al. THE EXTREMELY LONG-PERIOD X-RAY SOURCE IN A YOUNG SUPERNOVA REMNANT: A THORNE-ZYTKOW OBJECT DESCENDANT?[J]. ASTROPHYSICAL JOURNAL,2015,799(2).
APA Liu, XW.,Xu, RX.,van den Heuvel, EPJ.,Qiao, GJ.,Han, JL.,...&Li, XD.(2015).THE EXTREMELY LONG-PERIOD X-RAY SOURCE IN A YOUNG SUPERNOVA REMNANT: A THORNE-ZYTKOW OBJECT DESCENDANT?.ASTROPHYSICAL JOURNAL,799(2).
MLA Liu, XW,et al."THE EXTREMELY LONG-PERIOD X-RAY SOURCE IN A YOUNG SUPERNOVA REMNANT: A THORNE-ZYTKOW OBJECT DESCENDANT?".ASTROPHYSICAL JOURNAL 799.2(2015).

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来源：云南天文台

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