activity
20042024
most citedThe dynamical stability of W Ursae Majoris-type systems

110 citations · 823 across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.SR2024

Short-period Post-Common Envelope Binaries with Balmer Emission from SDSS and LAMOST Based on ZTF Photometric Data

Lifang Li, Fenghui Zhang

We present here 55 short period PCEBs containing a hot WD and a low-mass MS. Based on the photometric data from ZTF DR19, the light curves are analyzed for about 200 WDMS binaries…

astro-ph.EP2022★ 25 cited

Modeling H and He 10830 transmission spectrum of WASP-52b

Dongdong Yan, Kwang-il Seon, Jianheng Guo +2

Escaping atmosphere has been detected by the excess absorption of Ly, H and He triplet (10830) lines. Simultaneously modeling the absorption of the H and He 10830 li…

astro-ph.SR2022★ 17 cited

A Roche Lobe-filling hot Subdwarf and White Dwarf Binary: possible detection of an ejected common envelope

Jiangdan Li, Christopher A. Onken, Christian Wolf +12

Binaries consisting of a hot subdwarf star and an accreting white dwarf (WD) are sources of gravitational wave radiation at low frequencies and possible progenitors of type Ia supe…

astro-ph.SR2020★ 45 cited

LAMOST Medium-Resolution Spectroscopic Survey (LAMOST-MRS): Scientific goals and survey plan

Chao Liu, Jianning Fu, Jianrong Shi +38

Since September 2018, LAMOST starts a new 5-year medium-resolution spectroscopic survey (MRS) using bright/gray nights. We present the scientific goals of LAMOST-MRS and propose a…

astro-ph.SR2020★ 4 cited

Mass transfer of low-mass binaries and chemical anomalies among unevolved stars in globular clusters

Dandan Wei, Bo Wang, Xuefei Chen +3

While it is well known that mass transfer in binaries can pollute the surfaces of the accretors, it is still unclear whether this mechanism can reproduce the observed chemical inho…

astro-ph.SR2019★ 40 cited

Properties of Radial Velocities measurement based on LAMOST-II Medium-Resolution Spectroscopic Observations

R. Wang, A. -L. Luo, J. -J. Chen +28

The radial velocity (RV) is a basic physical quantity which can be determined through Doppler shift of the spectrum of a star. The precision of RV measurement depends on the resolu…