YNAO OpenIR  > 大样本恒星演化研究组
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
Liang XL(梁熙龙)1,2; Yoon, Suk-Jin2; Zhao, Jingkun3
发表期刊ASTRONOMICAL JOURNAL
2024-12-01
卷号168期号:6
DOI10.3847/1538-3881/ad87ec
产权排序第1完成单位
收录类别SCI
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.
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]
项目资助者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]
语种英语
学科领域天文学 ; 恒星与银河系
文章类型Article
出版者IOP Publishing Ltd
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-6256
URL查看原文
WOS记录号WOS:001359600800001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]OUTER LINDBLAD RESONANCE ; MILKY-WAY ; GALACTIC BAR ; SPIRAL STRUCTURE ; HERCULES STREAM ; DR2 LINKING ; DISK ; SIGNATURES ; ORIGIN ; SPACE
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文献类型期刊论文
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条目标识符http://ir.ynao.ac.cn/handle/114a53/27791
专题大样本恒星演化研究组
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, People's Republic of China;
2.Department of Astronomy & Center for Galaxy Evolution Research, Yonsei University, Seoul 03722, Republic of Korea; [email protected];
3.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People's Republic of China
第一作者单位中国科学院云南天文台
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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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