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Binary Population Synthesis
Han ZW(韩占文)1; Ge HW(葛宏伟)2; Chen XF(陈雪飞)3; Chen HL(陈海亮)4
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
2020-10-01
Volume20Issue:10Pages:14
DOI10.1088/1674-4527/20/10/161
Contribution Rank第1完成单位
Indexed BySCI
Keywordstars: evolution star: binaries (including multiple): close stars: statistics supernovae: general galaxies: stellar content methods: numerical
Abstract

In this review (which is similar to part of the review that I presented at the IAU meeting 266 Star Clusters - Basic Galactic Building Blocks throughout Time and Space at he GA in Rio 2009) I first summarize why binaries are key objects in the study of stellar populations, key objects to understand the evolution of star clusters, key objects to understand galaxies and thus the universe. I then focus on 3 specific topics: 1. the formation (via binaries) and evolution of very massive stars in dense clusters (like MUG 11 in M82) and the importance of stellar wind mass loss. 2. the evolution of the double neutron stars mergers in a starburst (the delayed time distribution of these mergers) and what this tells us about the suggestion that these mergers may be important production sites of r-process elements 3. the possible effect of massive binaries on the self-enrichment of globular clusters.

Funding ProjectNational Natural Science Foundation of China[11521303] ; National Natural Science Foundation of China[11733008] ; National Natural Science Foundation of China[11673058] ; National Natural Science Foundation of China[11703081] ; Key Research Programme of Frontier Sciences of the CAS[ZDBS-LY-7005]
Funding OrganizationNational Natural Science Foundation of China[11521303, 11733008, 11673058, 11703081] ; Key Research Programme of Frontier Sciences of the CAS[ZDBS-LY-7005]
Language英语
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
SubtypeArticle
PublisherNATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
Publication Place20A DATUN RD, CHAOYANG, BEIJING, 100012, PEOPLES R CHINA
ISSN1674-4527
URL查看原文
WOS IDWOS:000590254700001
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordCOMPACT OBJECT FORMATION ; SINGLE-DEGENERATE CHANNEL ; FINAL MASS RELATIONSHIP ; ACCRETING WHITE-DWARFS ; SUBDWARF-B-STARS ; X-RAY BINARIES ; EVOLUTIONARY SEQUENCES ; SPECTROSCOPIC BINARIES ; STELLAR EVOLUTION ; IA SUPERNOVAE
Citation statistics
Cited Times:2[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/23954
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
Corresponding AuthorHan ZW(韩占文)
Affiliation1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China
2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, China
3.University of the Chinese Academy of Sciences, Beijing 100049, China
4.Center for AstronomicalMega-Science, Chinese Academy of Sciences, Beijing 100101, China
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Corresponding Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Han ZW,Ge HW,Chen XF,et al. Binary Population Synthesis[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2020,20(10):14.
APA Han ZW,Ge HW,Chen XF,&Chen HL.(2020).Binary Population Synthesis.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,20(10),14.
MLA Han ZW,et al."Binary Population Synthesis".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 20.10(2020):14.
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