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Minimum accretion rate for millisecond pulsar formation in binary system
Pan,Yuanyue1,2; Zhang,Chengmin1; Wang,Na2
2013-02-21
Conference NameIAU Symposium 290:Feeding Compact Objects: Accretion on All Scales
Source PublicationFeeding Compact Objects: Accretion on All Scales, Proceedings of the International Astronomical Union, IAU Symposium 290
Volume290
Pages291-292
Conference Date20 - 24 August 2012
Correspondent Emailpanyuanyue@xao.ac.cn
Conference PlaceBeijing, China
PublisherCambridge University Press
Project Number2009CB824800 ; 2012CB821800 ; 10773017 ; 11173034 ; KJCX2-YW-T09
Contribution Rank2
Abstract

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.

Funding Organization973项目 ; IAU ; 973项目 ; IAU ; 国家自然科学基金 ; 国家自然科学基金 ; 中国科学院知识创新项目 ; 中国科学院知识创新项目
KeywordBinary System Millisecond Pulsar Accretion Rate
DOI10.1017/S1743921312020066
URL查看原文
Language英语
ISBN978-1-107-03379-5
Citation statistics
Document Type会议论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/985
Collection射电天文研究室_脉冲星研究团组
射电天文研究室
其它
Corresponding AuthorPan,Yuanyue
Affiliation1.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
2.Xinjiang Astronomical Observatories, Chinese Academy of Sciences, Xinjiang 830011, China
Recommended Citation
GB/T 7714
Pan,Yuanyue,Zhang,Chengmin,Wang,Na. Minimum accretion rate for millisecond pulsar formation in binary system[C]:Cambridge University Press,2013:291-292.
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