ANALYZING THE BINARY PULSARS ABOVE THE SPIN-UP LINE
文献类型：期刊论文
| 作者 | PAN, YUANYUE1,2 ; WANG, NA1; ZHANG, CHENGMIN2
|
| 刊名 | International Journal of Modern Physics: Conference Series
 |
| 出版日期 | 2013 |
| 卷号 | 23页码:111-114 |
| ISSN号 | 2010-1945 |
| DOI | 10.1142/s201019451301115x |
| 产权排序 | 1 |
| 英文摘要 | With accretion of mass from an evolving companion star, a neutron star can be spun up to an equilibrium period, which is set by the Kepler orbital period at the magnetosphere radius, expressed as a proportional relation between the spin period and magnetic field strength. The spin-up line relationship can be also expressed as a relation between period (P) and period derivative (Ṗ) for the pulsars with dipole radiation. All binary pulsars should lie below the spin-up line, if they accrete the sufficient masses from companions. So, we investigate the distribution of isolated and binary pulsars in the period (P) and magnetic field (B) diagram to see their positions relative to the spin-up line. It is found that the eight binary pulsars (of total 172) are above the spin-up line, thus we analyze their properties and present the possible process of their formations. |
| URL标识 | 查看原文 |
| 会议地点 | Beijing, China |
| 会议日期 | October 11–15, 2011 |
| 语种 | 英语 |
| 出版者 | World Scientific |
| 国家 | China |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/3185]  |
| 专题 | 脉冲星研究团组 |
| 通讯作者 | PAN, YUANYUE |
| 作者单位 | 1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Xinjiang 830011, China; 2.†National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China |
| 推荐引用方式 GB/T 7714 | PAN, YUANYUE,WANG, NA,ZHANG, CHENGMIN. ANALYZING THE BINARY PULSARS ABOVE THE SPIN-UP LINE[J]. International Journal of Modern Physics: Conference Series,2013,23:111-114. |
| APA | PAN, YUANYUE,WANG, NA,&ZHANG, CHENGMIN.(2013).ANALYZING THE BINARY PULSARS ABOVE THE SPIN-UP LINE.International Journal of Modern Physics: Conference Series,23,111-114. |
| MLA | PAN, YUANYUE,et al."ANALYZING THE BINARY PULSARS ABOVE THE SPIN-UP LINE".International Journal of Modern Physics: Conference Series 23(2013):111-114. |
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来源：新疆天文台
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