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Chinese Academy of Sciences Institutional Repositories Grid
Moving Groups in the Solar Neighborhood with Gaia, APOGEE, GALAH, and LAMOST: Dynamical Effects Gather Gas and the Ensuing Star Formation Plays an Important Role in Shaping the Stellar Velocity Distributions

文献类型:期刊论文

作者Liang XL(梁熙龙)2,3; Yoon, Suk-Jin2; Zhao, Jingkun1
刊名ASTRONOMICAL JOURNAL
出版日期2024-12-01
卷号168期号:6
ISSN号0004-6256
DOI10.3847/1538-3881/ad87ec
产权排序第1完成单位
文献子类Article
英文摘要With Gaia, APOGEE, GALAH, and LAMOST data, we investigate the positional, kinematic, chemical, and age properties of nine moving groups in the solar neighborhood. We find that each moving group has a distinct distribution in the velocity space in terms of its metallicity, alpha abundance, and age. Comparison of the moving groups with their underlying background stars suggests that they have experienced the enhanced, prolonged star formation. We infer that any dynamical effects that gathered stars as a moving group in the velocity space also worked for gas. We propose for the first time that the ensuing newborn stars from such gas inherited the kinematic feature from the gas, shaping the current stellar velocity distributions of the groups. Our findings improve the understanding of the origins and evolutionary histories of moving groups in the solar neighborhood.
学科主题天文学 ; 恒星与银河系
URL标识查看原文
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
WOS关键词OUTER LINDBLAD RESONANCE ; MILKY-WAY ; GALACTIC BAR ; SPIRAL STRUCTURE ; HERCULES STREAM ; DR2 LINKING ; DISK ; SIGNATURES ; ORIGIN ; SPACE
资助项目National Research Foundation of Korea[RS-2024-00344283]; National Research Foundation of Korea[2022R1A6A1A03053472]; National Natural Science Foundation of China[11988101]; National Natural Science Foundation of China[12273055]; National Natural Science Foundation of China[11927804]; Chinese Academy of Sciences[178GJHZ2022040GC]; The 2 m Chinese Space Station Telescope project; National Natural Science Foundation of China ( NSFC)[178GJHZ2022040GC]; National Natural Science Foundation of China ( NSFC)[12288102]; National Natural Science Foundation of China ( NSFC)[12125303]; National Natural Science Foundation of China ( NSFC)[12090040/3]; National Key R&D Program of China[2021YFA1600403]; Yunnan Fundamental Research Projects[202201BC070003]; International Centre of Supernovae; Yunnan Key Laboratory[202302AN360001]; Yunnan Revitalization Talent Support Program-Science & Technology Champion Project[202305AB350003]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001359600800001
出版者IOP Publishing Ltd
资助机构National Research Foundation of Korea[RS-2024-00344283, 2022R1A6A1A03053472] ; National Natural Science Foundation of China[11988101, 12273055, 11927804] ; Chinese Academy of Sciences[178GJHZ2022040GC] ; The 2 m Chinese Space Station Telescope project ; National Natural Science Foundation of China ( NSFC)[178GJHZ2022040GC, 12288102, 12125303, 12090040/3] ; National Key R&D Program of China[2021YFA1600403] ; Yunnan Fundamental Research Projects[202201BC070003] ; International Centre of Supernovae ; Yunnan Key Laboratory[202302AN360001] ; Yunnan Revitalization Talent Support Program-Science & Technology Champion Project[202305AB350003]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/27791]  
专题云南天文台_大样本恒星演化研究组
作者单位1.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People's Republic of China
2.Department of Astronomy & Center for Galaxy Evolution Research, Yonsei University, Seoul 03722, Republic of Korea; sjyoon0691@yonsei.ac.kr;
3.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, People's Republic of China;
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GB/T 7714
Liang XL,Yoon, Suk-Jin,Zhao, Jingkun. Moving Groups in the Solar Neighborhood with Gaia, APOGEE, GALAH, and LAMOST: Dynamical Effects Gather Gas and the Ensuing Star Formation Plays an Important Role in Shaping the Stellar Velocity Distributions[J]. ASTRONOMICAL JOURNAL,2024,168(6).
APA 梁熙龙,Yoon, Suk-Jin,&Zhao, Jingkun.(2024).Moving Groups in the Solar Neighborhood with Gaia, APOGEE, GALAH, and LAMOST: Dynamical Effects Gather Gas and the Ensuing Star Formation Plays an Important Role in Shaping the Stellar Velocity Distributions.ASTRONOMICAL JOURNAL,168(6).
MLA 梁熙龙,et al."Moving Groups in the Solar Neighborhood with Gaia, APOGEE, GALAH, and LAMOST: Dynamical Effects Gather Gas and the Ensuing Star Formation Plays an Important Role in Shaping the Stellar Velocity Distributions".ASTRONOMICAL JOURNAL 168.6(2024).

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来源:云南天文台

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