activity
20162022
most citedGD424 -- a helium-atmosphere white dwarf with a large amount of trace hydrogen in the process of digesting a rocky planetesimal

28 citations · 70 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2022

LTD064402+245919, compact binary or subgiant with red star eclipsing binary?

Jincheng Guo, Cheng Liu

Recently, a single-line spectroscopic binary, LTD064402+245919, has been discovered by Yang et al. Using data from LAMOST and ZTF, the unseen companion is estimated to have a mass…

astro-ph.EP202028 cited

GD424 -- a helium-atmosphere white dwarf with a large amount of trace hydrogen in the process of digesting a rocky planetesimal

Paula Izquierdo, Odette Toloza, Boris T. Gänsicke +5

The photospheric metal pollution of white dwarfs is now well-established as the signature of the accretion of planetary debris. However, the origin of the trace hydrogen detected i…

astro-ph.SR202026 cited

A Catalog of RV Variable Star Candidates from LAMOST

Zhijia Tian, Xiaowei Liu, Haibo Yuan +14

RV variable stars are important in astrophysics. The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) spectroscopic survey has provided ~ 6.5 million stellar spec…

astro-ph.SR2019

A New Luminous blue variable in the outskirt of the Andromeda Galaxy

Yang Huang, Huaiwei Zhang, Chun Wang +8

The hot massive luminous blue variables (LBVs) represent an important evolutionary phase of massive stars. Here, we report the discovery of a new LBV -- LAMOST J0037+4016 in the di…

astro-ph.SR20193 cited

X-ray Activity from Different Types of Stars

Lin He, Song Wang, Xiaojie Xu +10

X-ray emission is an important indicator of stellar activity. In this paper, we study stellar X-ray activity using the XMM-Newton and LAMOST data for different types of stars. We p…

astro-ph.SR201813 cited

A Combined Chandra and LAMOST Study of Stellar Activity

Lin He, Song Wang, Jifeng Liu +5

We probed stellar X-ray activity over a wide range of stellar parameters, using {\it Chandra} and LAMOST data. We measured the X-ray-to-bolometric luminosity ratio ($R_X = L_X/L_{\…