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![]() |
刊名 | ASTRONOMICAL JOURNAL
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出版日期 | 2024-12-01 |
卷号 | 168期号:6 |
ISSN号 | 0004-6256 |
DOI | 10.3847/1538-3881/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; |
推荐引用方式 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). |
入库方式: OAI收割
来源:云南天文台
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