NAOC Open IR
fast脉冲星发现新视野
张承民1; 王培2; 杨佚沿3
2017
Source Publication科技导报北京
ISSN1000-7857
Volume035Issue:021Pages:12
Abstract1脉冲星的特性与科学意义 脉冲星是旋转的中子星,其质量约为一个太阳而半径只有10 km,它是大质量恒星生命终结并经历超新星爆发的产物,此星体在1967年首先被英国天文学家乔瑟琳·贝尔发现,堪称20世纪四大天文学发现之一。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/39395
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.中国科学院大学
3.北京师范大学
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
张承民,王培,杨佚沿. fast脉冲星发现新视野[J]. 科技导报北京,2017,035(021):12.
APA 张承民,王培,&杨佚沿.(2017).fast脉冲星发现新视野.科技导报北京,035(021),12.
MLA 张承民,et al."fast脉冲星发现新视野".科技导报北京 035.021(2017):12.
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