中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Minimum accretion rate for millisecond pulsar formation in binary system

文献类型:会议论文

作者Pan,Yuanyue1,2; Zhang,Chengmin1; Wang,Na2
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

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