Binary stars in the new millennium

doi:10.1016/j.ppnp.2023.104083

	Binary stars in the new millennium
	Chen XF(陈雪飞)3; Liu ZW(柳正伟)3; Han ZW(韩占文)3
刊名	PROGRESS IN PARTICLE AND NUCLEAR PHYSICS
	2024-01
卷号	134
关键词	Binary stars Population synthesis Binary mass transfer Common envelope Nucleosynthesis
ISSN号	0146-6410
DOI	10.1016/j.ppnp.2023.104083
产权排序	第1完成单位
文献子类	Review
英文摘要	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.
学科主题	天文学
URL标识	查看原文
出版地	RADARWEG 29, 1043 NX AMSTERDAM, NETHERLANDS
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]
WOS关键词	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
WOS研究方向	Physics
语种	英语
出版者	ELSEVIER
WOS记录号	WOS:001133858900001
资助机构	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]
内容类型	期刊论文
版本	出版稿
源URL	[http://ir.ynao.ac.cn/handle/114a53/26514]
专题	云南天文台_大样本恒星演化研究组
作者单位	1.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, CAS, Kunming 650216, China; 3.Yunnan Observatories, the Chinese Academy of Sciences, Kunming, 650296, China;
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).