activity
20092025
most citedStellar activity with LAMOST - II. Chromospheric activity in open clusters

70 citations · 472 across the 20 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

10 papers · 1 filter

astro-ph.GA2022★ 7 cited

Revisit NGC 5466 Tidal Stream with , SDSS/SEGUE and LAMOST

Yong Yang, Jing-Kun Zhao, Miho N. Ishigaki +5

By mining the data from EDR3, SDSS/SEGUE DR16 and LAMOST DR8, 11 member stars of the NGC 5466 tidal stream are detected and 7 of them are newly identified. To reject contami…

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.GA2021★ 2 cited

Partitioning the Galactic Halo with Gaussian Mixture Models

Xilong Liang, Yuqin Chen, Jingkun Zhao +1

The Galactic halo is supposed to form from merging with nearby dwarf galaxies. In order to probe different components of the Galactic halo, we have applied the Gaussian Mixture Mod…

astro-ph.GA2020★ 2 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★ 1 cited

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.GA2020★ 30 cited

Is NGC 5824 the Core of the Progenitor of the Cetus Stream?

Jiang Chang, Zhen Yuan, Xiang-Xiang Xue +5

A large number of new members (150) of the Cetus Stream (CS) were identified from their clustering features in dynamical space using 6D kinematic data by combining LAMOST DR5…

astro-ph.GA2019★ 12 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.GA2019★ 2 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…

astro-ph.GA2018★ 8 cited

On the radial metallicity gradient and radial migration effect of the Galactic disk

Yunpeng Jia, Yuqin Chen, Gang Zhao +4

We study the radial metallicity gradient as a function of [Mg/Fe] and with the help of a guiding radius based on the Apache Point Observatory Galactic Evolution…

astro-ph.GA2009★ 55 cited

A Catalog of Moving Group Candidates in The Solar Neighborhood

Jingkun Zhao, Gang Zhao, Yuqin Chen

Based on the kernel estimator and wavelet technique, we have identified 22 moving group candidates in the solar neighborhood from a sample which includes around 14,000 dwarfs and 6…