Chengqun Yang
0000-0003-1972-0086
5 papers found
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Tracing Kinematic and Chemical Properties of Sagittarius Stream by K-Giants, M-Giants, and BHB stars
Identifying Galactic Halo Substructure in 6D Phase Space Using ∼13,000 LAMOST K Giants
Galactic Rotation and the Oort Constants in the Solar Vicinity
Anisotropy of the Milky Way’s Stellar Halo Using K Giants from LAMOST andGaia
Flare and Warp of Galactic Disk with OB Stars fromGaiaDR2
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