NAOC Open IR
脉冲星参数统计和演化
蔡炎; 阿里塔尼; 赵永恒; 张承民
2011
Source Publication天文学报
ISSN0001-5245
Volume052Issue:006Pages:449
Abstract统计分析了目前发现的几种脉冲星的自转周期和表面磁场以及空间的分布情况,揭示出毫秒脉冲星比普通射电脉冲星、LMXB(低质量X射线双星)比HMXB(高质量X射线双星)的空间分布要更加弥散;孤立毫秒脉冲星自转周期分布的峰值为4.7ms,而普通脉冲星的相应值为0.6S,双星中毫秒脉冲星这一值为3.5ms;FERMI脉冲星(Fermi Gamma-ray Space Telescope发现的伽玛射线脉冲星)和正常脉冲星磁场集中于1012Gs;某些年轻的高能脉冲星与超新星遗迹关联.另外结合脉冲星形成演化模型,对这些分布特点进行了一定的说明.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/40522
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
蔡炎,阿里塔尼,赵永恒,等. 脉冲星参数统计和演化[J]. 天文学报,2011,052(006):449.
APA 蔡炎,阿里塔尼,赵永恒,&张承民.(2011).脉冲星参数统计和演化.天文学报,052(006),449.
MLA 蔡炎,et al."脉冲星参数统计和演化".天文学报 052.006(2011):449.
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