activity
20152021
most citedMapping the Milky Way with LAMOST III: Complicated spatial structure in the outer disc

77 citations · 281 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2021★ 44 cited

The Spectroscopic Binaries from LAMOST Medium-Resolution Survey (MRS). I. Searching for Double-lined Spectroscopic Binaries (SB2s) with Convolutional Neural Network

Bo Zhang, Ying-Jie Jing, Fan Yang +13

We developed a convolutional neural network (CNN) model to distinguish the double-lined spectroscopic binaries (SB2s) from others based on single exposure medium-resolution spectra…

astro-ph.GA2018★ 77 cited

Mapping the Milky Way with LAMOST III: Complicated spatial structure in the outer disc

Hai-Feng Wang, Chao Liu, Yan Xu +2

We present {complexity} of the Galactic outer disc {by fitting the stellar volume densities of the red giant branch stars with a two-disc component model}. {The discs are confirmed…

astro-ph.GA2017★ 5 cited

Rediscovering the Galactic outer disk with LAMOST data

Chao Liu, Yan Xu, Haifeng Wang +1

From the derived stellar density profile using LAMOST giant stars, we find that the Galactic disk does not show truncation or break, but smoothly transit to the halo from 19 kpc. T…

astro-ph.GA2017★ 24 cited

The peculiar in-plane velocities in the outer disc of the Milky Way

Hai-Jun Tian, Chao Liu, Jun-Chen Wan +9

We present the peculiar in-plane velocities derived from the LAMOST red clump stars, which are purified and separated by a novel approach into two groups with different ages. The s…

astro-ph.GA2017★ 18 cited

Red Clump stars from LAMOST II: the outer disc of the Milky Way

Jun-chen Wan, Chao Liu, Li-cai Deng +1

We present stellar density maps of the Galactic outer disc with red clump stars from the LAMOST data. These samples are separated into younger (mean age ~ 2.7 Gyr) and older (mean…

astro-ph.GA2017★ 5 cited

The age-kinematical features in the Milky Way outer disk

Chao Liu, Hai-Jun Tian, Jun-Chen Wan

We derive the mean velocity components at various Galactocentric radii from 8 to 14 kpc using about 40,000 red clump stars observed in the LAMOST survey. We find that the vertical…