KMS National Astronomical Observatories, CAS
A New Moving Group in the Local Arm | |
Liang, Xilong1,2; Zhao, Jingkun1,2; Chen, Yuqin1,2; Fang, Xiangsong1; Ye, Xianhao1,2; Zhang, Jiajun1,2; Kong, Xiaoming3; Zhao, Gang1,2 | |
2020-05-01 | |
Source Publication | ASTRONOMICAL JOURNAL
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ISSN | 0004-6256 |
Volume | 159Issue:5Pages:9 |
Abstract | We present a new moving group clustered in kinematics, spatial position, and elemental abundances. Its spatial position is around the center of the Local Arm of the Milky Way. A convergent point method was taken to select candidate member stars. Among 206 candidate member stars, 74 are pre-main-sequence stars and some of them have stellar disks. We presume those pre-main-sequence stars belong to the Orion nebula. We suggest that this moving group is caused by the density wave of the Local Arm passing by. |
Keyword | Galaxy kinematics Stellar associations Galaxy abundances |
Funding Organization | National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key R&D Program of China ; National Key R&D Program of China ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key R&D Program of China ; National Key R&D Program of China ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key R&D Program of China ; National Key R&D Program of China ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key R&D Program of China ; National Key R&D Program of China ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; National Development and Reform Commission ; National Development and Reform Commission |
DOI | 10.3847/1538-3881/ab7fa9 |
WOS Keyword | YOUNG ; KINEMATICS ; HYADES ; STARS ; ASSOCIATIONS ; ABUNDANCES ; CLUSTER ; STREAM |
Language | 英语 |
Funding Project | National Natural Science Foundation of China[11988101] ; National Natural Science Foundation of China[11973048] ; National Natural Science Foundation of China[11927804] ; National Natural Science Foundation of China[11890694] ; National Natural Science Foundation of China[11625313] ; National Natural Science Foundation of China[11803016] ; National Key R&D Program of China[2019YFA0405502] ; Astronomical Big Data Joint Research Center ; National Development and Reform Commission |
Funding Organization | National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key R&D Program of China ; National Key R&D Program of China ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key R&D Program of China ; National Key R&D Program of China ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key R&D Program of China ; National Key R&D Program of China ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key R&D Program of China ; National Key R&D Program of China ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; National Development and Reform Commission ; National Development and Reform Commission |
WOS Research Area | Astronomy & Astrophysics |
WOS Subject | Astronomy & Astrophysics |
WOS ID | WOS:000525675200001 |
Publisher | IOP PUBLISHING LTD |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.bao.ac.cn/handle/114a11/56174 |
Collection | 中国科学院国家天文台 |
Corresponding Author | Zhao, Jingkun |
Affiliation | 1.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China 2.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China 3.Shangdong Univ Weihai, Sch Mech Elect & Informat Engn, Weihai 264209, Peoples R China |
Recommended Citation GB/T 7714 | Liang, Xilong,Zhao, Jingkun,Chen, Yuqin,et al. A New Moving Group in the Local Arm[J]. ASTRONOMICAL JOURNAL,2020,159(5):9. |
APA | Liang, Xilong.,Zhao, Jingkun.,Chen, Yuqin.,Fang, Xiangsong.,Ye, Xianhao.,...&Zhao, Gang.(2020).A New Moving Group in the Local Arm.ASTRONOMICAL JOURNAL,159(5),9. |
MLA | Liang, Xilong,et al."A New Moving Group in the Local Arm".ASTRONOMICAL JOURNAL 159.5(2020):9. |
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