activity
20242026
collaborators

10 papers

astro-ph.SR2026

Identification of false positive double-lined spectroscopic binaries in LAMOST-MRS data due to moonlight contamination

Zhoulin Wang, Mikhail Kovalev, Jianping Xiong +2

We present a method for identifying false positive double-lined spectroscopic binary (SB2) candidates by analysing medium-resolution survey spectra from the Large Sky Area Multi-Ob…

astro-ph.SR2025

A New Algol-type Binary with an Accretion disk

Tongyu He, Jiao Li, Xiaobin Zhang +10

We present a comprehensive photometric and spectroscopic analysis of the Algol-type binary \textit{Gaia} DR3 1892576067672499328. We identified the system as a spectroscopic binary…

astro-ph.SR2025

Fundamental Parameters for Totally Eclipsing Contact Binaries Observed by TESS

Xu Ding, KaiFan Ji, ZhiMing Song +5

Totally eclipsing contact binaries provide a unique opportunity to accurately determine mass ratios through photometric methods alone, eliminating the need for spectroscopic data.…

astro-ph.GA2025

The Initial Mass Function of the Galactic Early-type Field Stars Based on the LAMOST Survey

Qida Li, Jianping Xiong, Zhenwei Li +4

Research on the high-mass end of the initial mass function (IMF) has been limited due to a scarcity of samples. Recently, Large Sky Area Multi-Object Fiber Spectroscopic Telescope…

astro-ph.SR2025

Orbital Parameters of 665 Double-lined Spectroscopic Binaries in the LAMOST Medium-Resolution Survey

Sufen Guo, Mikhail Kovalev, Jiao Li +9

The period, mass ratio, eccentricity, and other orbital parameters are fundamental for investigating binary star evolution. However, the number of binaries with known orbital param…

astro-ph.SR2025

Mass, Luminosity, and Stellar Age of Early-type Stars from the LAMOST Survey

Qida Li, Jianping Xiong, Jiao Li +4

Mass () and luminosity () are fundamental parameters of stars but can only be measured indirectly. Typically, effective temperature (), surface gravity (${\rm lo…