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Seven pulsars in binary systems above the spin-up line

文献类型:会议论文

作者Pan,Y.Y.; Wang,N.
出版日期2013-02-21
会议名称IAU Symposium 291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years
会议日期20-31 August 2012
会议地点Beijing, China
通讯作者邮箱panyuanyue@xao.ac.cn
关键词Pulsar binary spin-up line
卷号291
页码462-464
通讯作者Pan, Y. Y.
英文摘要Using data from the ATNF pulsar catalogue, 186 binary pulsars are shown in the magnetic field versus spin period (B-P) diagram, and their relationship to the spin-up line is investigated. Generally speaking, pulsars in binary systems should be below the spin-up line when they get enough accretion mass from their companions. It is found that there are seven binary pulsars above the spin-up line. Based on the parameters of these seven binary systems, we describe possible reasons why they are above the spin-up line.
会议主办者IAU
会议网址http://www.pulsarastronomy.net/IAUS291/
会议录Neutron Stars and Pulsars: Challenges and Opportunities after 80 years, Proceedings of the International Astronomical Union, IAU Symposium 291
会议录出版者Cambridge University Press
语种英语
ISBN号978-1-107-03380-1
源URL[http://ir.xao.ac.cn/handle/45760611-7/984]  
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Xinjiang Astronomical Observatory, CAS, Urumqi 830011, China
推荐引用方式
GB/T 7714
Pan,Y.Y.,Wang,N.. Seven pulsars in binary systems above the spin-up line[C]. 见:IAU Symposium 291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years. Beijing, China. 20-31 August 2012.http://www.pulsarastronomy.net/IAUS291/.

入库方式: OAI收割

来源:新疆天文台

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