YNAO OpenIR  > 大样本恒星演化研究组
双中子星的星族合成研究
Alternative TitlePopulation synthesis of double neutron stars
陈海亮1,2,3; 陈雪飞1,2,3; 韩占文1,2,3
Source Publication物理(Physics)
2019
Volume48Issue:9Pages:561-566
DOI10.7693/wl20190903
ClassificationP145.6
Contribution Rank第1完成单位
Indexed By核心
Keyword双星 星族合成 双中子星 引力波
Abstract

双中子星是天体物理中重要的研究对象,对于许多研究领域都有重要作用。2017年LIGO/Virgo发现第一个双中子星并合事件GW170817,开启了用引力波探测发现双中子星的序幕。文章主要介绍了双中子星的双星演化通道,以及双中子星星族合成的一些性质。此外,还介绍了双星演化中的一些不确定性以及形成GW170817双中子星的双星演化通道。 

Other Abstract

Double neutron stars are important objects in astrophysics and very important for many scientific studies. In 2017, LIGO/Virgo first discovered gravitational waves from the double neutron star merger GW170817, indicating a new method of discovering these stars. In this paper we shall describe the isolated binary formation scenario of double neutron stars and the properties of their populations. In addition, we discuss the binary formation channel for the GW170817 merger and some uncertainties in binary evolution, which are important for the formation of binary neutron stars.

Funding ProjectN/A
Funding OrganizationN/A
Language中文
Subject Area天文学 ; 恒星与银河系 ; 恒星形成与演化
MOST Discipline Catalogue理学 ; 理学::天文学
ISSN0379-4148
Citation statistics
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/20882
Collection大样本恒星演化研究组
中国科学院天体结构与演化重点实验室
Affiliation1.中国科学院云南天文台, 昆明, 650011
2.中国科学院天体结构与演化重点实验室, 昆明, 650011
3.中国科学院天文大科学研究中心, 北京, 100012
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
陈海亮,陈雪飞,韩占文. 双中子星的星族合成研究[J]. 物理(Physics),2019,48(9):561-566.
APA 陈海亮,陈雪飞,&韩占文.(2019).双中子星的星族合成研究.物理(Physics),48(9),561-566.
MLA 陈海亮,et al."双中子星的星族合成研究".物理(Physics) 48.9(2019):561-566.
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