Mapping the Galactic Disk with the LAMOST and Gaia Red Clump Sample. VIII. Mapping the Kinematics of the Galactic Disk Using Mono-age and Mono-abundance Stellar Populations

We present a comprehensive study of the kinematic properties of the different Galactic disk populations, as defined by the chemical abundance ratios and stellar ages, across a large disk volume (4.5 ≤ R ≤ 15.0 kpc and ∣ Z ∣ ≤ 3.0 kpc), by using the LAMOST-Gaia red clump sample stars. We determine th...

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書誌詳細

主要な著者:	Weixiang Sun, Yang Huang, Han Shen, Chun Wang, Huawei Zhang, Zhijia Tian, Xiaowei Liu, Biwei Jiang
フォーマット:	Artigo
言語:	Inglês
出版事項:	IOP Publishing 2024-01-01
シリーズ:	The Astrophysical Journal
主題:	Stellar abundances Stellar kinematics Stellar populations Milky Way formation Milky Way evolution Milky Way disk
オンライン･アクセス:	https://doi.org/10.3847/1538-4357/ad06ad
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