activity
20172021
most citedStellar chromospheric activity and age relation from open clusters in the LAMOST Survey

32 citations · 78 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2021

High-α-Metal-Rich stars in the LAMOST-MRS survey and its connection with the galactic bulge

Haopeng Zhang, Yuqin Chen, Gang Zhao +6

We report the detection of a large sample of high--metal-rich stars on the low giant branch with dex in the LAMOST-MRS survey. This special group corresponds to a…

astro-ph.GA20202 cited

Nearly 30,000 late-type main-sequence stars with stellar age from LAMOST DR5

Jiajun Zhang, Jingkun Zhao, Terry D. Oswalt +3

We construct a sample of nearly 30,000 main-sequence stars with 4500K 5000K and stellar ages estimated by the chromospheric activityage relation. This sample is u…

astro-ph.GA2020

A new moving group in the Local Arm

Xilong Liang, Jingkun Zhao, Yuqin Chen +5

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 con…

astro-ph.GA201912 cited

Elemental abundances distributions in (R, ) plane with LAMOST DR5 and Gaia DR2

Xilong Liang, Jingkun Zhao, Yuqin Chen +4

Since Gaia DR2 was released, many velocity structures in the disk have been revealed such as large scale ridge-like patterns in the phase space. Both kinematic information and stel…

astro-ph.SR201932 cited

Stellar chromospheric activity and age relation from open clusters in the LAMOST Survey

Jiajun Zhang, Jingkun Zhao, Terry D. Oswalt +5

We identify member stars of more than 90 open clusters in the LAMOST survey. With the method of Fang et al.(2018), the chromospheric activity (CA) indices logR'CaK for 1091 member…

astro-ph.GA20192 cited

A Hint of Three-section Halo as Seen from the APOGEE DR14

Y. Q. Chen, G. Zhao, X. X. Xue +4

Based on the [Fe/H] versus [Mg/Fe] diagram and distances from APOGEE data release 14, we compare the spatial distributions, the l-Vlos diagram and the abundance gradients between h…