activity
20122025
most citedPhysical Properties and Catalogue of EW-type Eclipsing Binaries Observed by LAMOST

157 citations · 239 across the 17 of their papers we have counts for

collaborators

26 papers

astro-ph.SR2025

Tidally Trapped Two-pole Pulsations Discovered in a Close Binary with a Massive Cephei Star

Ping Li, Wen-Ping Liao, Sheng-Bang Qian +4

Tidally tilted pulsators (TTPs), whose pulsation axis aligns with the binary's semi-major axis, represent a newly established class of oscillators in binary systems. While all prev…

astro-ph.SR2025

Orbital and Pulsation Analysis of 42 Heartbeat Stars Discovered in TESS Data

Min-Yu Li, Sheng-Bang Qian, Ai-Ying Zhou +7

Heartbeat stars (HBSs) are ideal laboratories for studying the formation and evolution of binary stars in eccentric orbits and their mutual tidal interactions. We present 42 new HB…

astro-ph.SR2025

V455 Car: an oscillating eclipsing Algol-type binary in triple star system

Zhao-Long Deng, Wen-Ping Liao, Li-Ying Zhu +3

V455 Car is a southern oscillating eclipsing Algol-type system with an orbital period of 5.132888 days. Our first photometric solutions based on the Transiting Exoplanet Survey Sat…

astro-ph.SR2025

Heartbeat Stars Recognition Based on Recurrent Neural Networks: Method and Validation

Min-Yu Li, Sheng-Bang Qian, Li-Ying Zhu +7

Since the variety of their light curve morphologies, the vast majority of the known heartbeat stars (HBSs) have been discovered by manual inspection. Machine learning, which has al…

astro-ph.EP2025

Comprehensive Parameter Determination of Exoplanet through Asteroseismic Host Star Constraints

Wen-Xu Lin, Sheng-Bang Qian, Li-Ying Zhu +5

This study develops a robust framework for exoplanet characterization by leveraging asteroseismic constraints on host stars. Using precise photometric data from missions such as \t…

astro-ph.SR20245 cited

Observational Properties of 155 Cephei pulsating variable stars

Xiang-dong Shi, Sheng-bang Qian, Li-ying Zhu +3

Cephei pulsating variable (BCEP) stars are the most massive pulsating variable stars in the main sequence, exhibiting both p- and g-mode pulsations. In this study, we identifie…