Minimum accretion rate for millisecond pulsar formation in binary system
文献类型:会议论文
作者 | Pan,Yuanyue1,2![]() ![]() |
出版日期 | 2013-02-21 |
会议名称 | IAU Symposium 290:Feeding Compact Objects: Accretion on All Scales |
会议日期 | 20 - 24 August 2012 |
会议地点 | Beijing, China |
通讯作者邮箱 | panyuanyue@xao.ac.cn |
关键词 | Binary system millisecond pulsar accretion rate |
卷号 | 290 |
页码 | 291-292 |
通讯作者 | Pan, Y. Y. |
英文摘要 | 186 binary pulsars are shown in the magnetic field versus spin period (B-P) diagram, and their relations to the millisecond pulsars can be clearly seen. We declaim a minimum accretion rate for the millisecond pulsar formation both from the observation and theory. If the accretion rate is lower than the minimum accretion rate, the pulsar in binary system will not become a millisecond pulsar after the evolution. |
会议主办者 | IAU |
会议网址 | http://iaus290.bao.ac.cn/ |
会议录 | Feeding Compact Objects: Accretion on All Scales, Proceedings of the International Astronomical Union, IAU Symposium 290
![]() |
会议录出版者 | Cambridge University Press |
语种 | 英语 |
ISBN号 | 978-1-107-03379-5 |
源URL | [http://ir.xao.ac.cn/handle/45760611-7/985] ![]() |
专题 | 脉冲星研究团组 新疆天文台_射电天文研究室 新疆天文台_其它 |
作者单位 | 1.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China 2.Xinjiang Astronomical Observatories, Chinese Academy of Sciences, Xinjiang 830011, China |
推荐引用方式 GB/T 7714 | Pan,Yuanyue,Zhang,Chengmin,Wang,Na. Minimum accretion rate for millisecond pulsar formation in binary system[C]. 见:IAU Symposium 290:Feeding Compact Objects: Accretion on All Scales. Beijing, China. 20 - 24 August 2012.http://iaus290.bao.ac.cn/. |
入库方式: OAI收割
来源:新疆天文台
浏览0
下载0
收藏0
其他版本
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。