Binary stars in the new millennium

doi:10.1016/j.ppnp.2023.104083

YNAO OpenIR > 大样本恒星演化研究组

	Binary stars in the new millennium
	Chen XF(陈雪飞)1 ; Liu ZW(柳正伟)1 ; Han ZW(韩占文)1
发表期刊	PROGRESS IN PARTICLE AND NUCLEAR PHYSICS
	2024-01
卷号	134
DOI	10.1016/j.ppnp.2023.104083
产权排序	第1完成单位
收录类别	SCI ; EI
关键词	Binary stars Population synthesis Binary mass transfer Common envelope Nucleosynthesis
摘要	Binary stars are as common as single stars. Binary stars are of immense importance astrophysicists because that they allow us to determine the masses of the stars independent of their distances. They are the cornerstone of the understanding of stellar evolutionary theory and play an essential role in cosmic distance measurement, galactic evolution, nucleosynthesis and the formation of important objects such as cataclysmic variable stars, X-ray binaries, Type Ia supernovae, and gravitational wave-producing double compact objects. In this article, review the significant theoretical and observational progresses in addressing binary stars the new millennium. Increasing large survey projects have led to the discovery of enormous numbers of binary stars, which enables us to conduct statistical studies of binary populations, and therefore provide unprecedented insight into the stellar and binary evolution physics. Meanwhile, the rapid development of theoretical concepts and numerical approaches for binary evolution have made a substantial progress on the alleviation of some long-standing binary related problems such as the stability of mass transfer and common envelope evolution. Nevertheless, it remains a challenge to have a full understanding of fundamental problems of stellar and binary astrophysics. The upcoming massive survey projects and increasingly sophisticated computational methods will lead to future progress.
资助项目	National Natural Science Foundation of China (NSFC)[12125303]; National Natural Science Foundation of China (NSFC)[12288102]; National Natural Science Foundation of China (NSFC)[12090040/3]; National Key R and D Program of China[2021YFA1600403/1]; National Key R and D Program of China[2021YFA1600400]; Natural Science Foundation of Yunnan Province[202201BC070003]; Natural Science Foundation of Yunnan Province[202001AW070007]; International Centre of Supernovae, Yunnan Key Laboratory[202302AN360001]; Yunnan Revitalization Talent Support Program-Science and Technology Champion Project[202305AB350003]
项目资助者	National Natural Science Foundation of China (NSFC)[12125303, 12288102, 12090040/3] ; National Key R and D Program of China[2021YFA1600403/1, 2021YFA1600400] ; Natural Science Foundation of Yunnan Province[202201BC070003, 202001AW070007] ; International Centre of Supernovae, Yunnan Key Laboratory[202302AN360001] ; Yunnan Revitalization Talent Support Program-Science and Technology Champion Project[202305AB350003]
语种	英语
学科领域	天文学
文章类型	Review
出版者	ELSEVIER
出版地	RADARWEG 29, 1043 NX AMSTERDAM, NETHERLANDS
ISSN	0146-6410
URL	查看原文
WOS记录号	WOS:001133858900001
WOS研究方向	Physics
WOS类目	Physics, Nuclear ; Physics, Particles & Fields
关键词[WOS]	COMMON-ENVELOPE BINARIES ; METAL-POOR STARS ; ASYMPTOTIC GIANT BRANCH ; DOUBLE-CORE EVOLUTION ; DOUBLE WHITE-DWARFS ; X-RAY BINARIES ; ROCHE-LOBE OVERFLOW ; R-PROCESS NUCLEOSYNTHESIS ; MASS-RATIO DISTRIBUTION ; MAIN-SEQUENCE BINARIES
EI入藏号	20234815131653
EI主题词	Mass transfer
EI分类号	641.3 Mass Transfer - 657.2 Extraterrestrial Physics and Stellar Phenomena - 721.1 Computer Theory, Includes Formal Logic, Automata Theory, Switching Theory, Programming Theory - 804 Chemical Products Generally - 931.5 Gravitation, Relativity and String Theory
引用统计	被引频次：11[WOS] [WOS记录] [WOS相关记录]
文献类型	期刊论文
版本	出版稿
条目标识符	http://ir.ynao.ac.cn/handle/114a53/26514
专题	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
作者单位	1.Yunnan Observatories, the Chinese Academy of Sciences, Kunming, 650296, China; 2.Key Laboratory for the Structure and Evolution of Celestial Objects, CAS, Kunming 650216, China; 3.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, China
第一作者单位	中国科学院云南天文台
推荐引用方式 GB/T 7714	Chen XF,Liu ZW,Han ZW. Binary stars in the new millennium[J]. PROGRESS IN PARTICLE AND NUCLEAR PHYSICS,2024,134.
APA	陈雪飞,柳正伟,&韩占文.(2024).Binary stars in the new millennium.PROGRESS IN PARTICLE AND NUCLEAR PHYSICS,134.
MLA	陈雪飞,et al."Binary stars in the new millennium".PROGRESS IN PARTICLE AND NUCLEAR PHYSICS 134(2024).

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