activity
20242026
collaborators

13 papers

astro-ph.SR2026

Surface brightness-color relations for red giant branch stars: Observational constraints on metallicity effects using the ARD method

Jianping Xiong, Xiaodian Chen, Jiao Li +5

Aims: We aim to quantify the metallicity dependence of the SBCR for red giant branch (RGB) stars and to test the robustness of the relation using asteroseismic radii, Gaia distance…

astro-ph.SR2026

Empirical colour--effective temperature relations in the SDSS system from IRFM temperatures of GALAH and APOGEE stars

Zenghua Zhou, Luca Casagrande, Xiaobin Zhang +5

Reliable estimates of stellar effective temperature () are fundamental to stellar population studies and Galactic astrophysics. However, the majority of stars ob…

astro-ph.SR2026

Stellar Parameters and Orbital Period Estimates for Composite-Spectrum sdB+MS Binaries from LAMOST

Jiangdan Li, Jianping Xiong, Jiao Li +5

Hot subdwarf (sdB) stars in binary systems with main-sequence (MS) companions provide valuable insights into mass transfer and envelope ejection processes in binary evolution. Thei…

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.…