activity
20102026
most citedThe most plausible explanation of the cyclical period changes in close binaries: the case of the RS CVn-type binary WW Dra

124 citations · 317 across the 30 of their papers we have counts for

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Showing 2024Show all

13 papers · 1 filter

astro-ph.EP2024★ 1 cited

Decoding the Future of Exoplanets: Asteroseismic Confirmation of Subgiant and Red Giant Hosts

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

Asteroseismology has emerged as a powerful tool to unravel the intricate relationships between evolved stars and their planetary systems. In this study, we leverage this technique…

astro-ph.SR2024★ 3 cited

CZ Aqr: an oscillating eclipsing Algol-type system composed of a Sct primary star and a subgiant star in a quadruple system

Qi-Huan Zeng, Wen-Ping Liao, Sheng-Bang Qian +3

Eclipsing Algol-type systems containing a Scuti (hereafter Sct) star enable precise determination of physical parameters and the investigation of stellar internal structure…

astro-ph.SR2024

Evolutionary states and triplicity of four massive semi-detached binaries with long-term decreasing orbital periods in the LMC

Fu-Xing Li, Sheng-Bang Qian, Li-ying Zhu +6

The massive semi-detached binary with a long-term decreasing orbital period may involve a rapid mass-transfer phase in Case A, and thus they are good astrophysical laboratories for…

astro-ph.SR2024

Five New Heartbeat Star Systems with Tidally Excited Oscillations Discovered Based on TESS Data

Min-Yu Li, Sheng-Bang Qian, Ai-Ying Zhou +6

Heartbeat stars (HBSs) with tidally excited oscillations (TEOs) are ideal astrophysical laboratories for studying the internal properties of the systems. In this paper, five new HB…

astro-ph.SR2024★ 3 cited

Twenty-three New Heartbeat Star Systems Discovered Based on TESS Data

Min-Yu Li, Sheng-Bang Qian, Ai-Ying Zhou +6

Heartbeat stars (HBSs) are ideal astrophysical laboratories to study the formation and evolution of binary stars in eccentric orbits and the internal structural changes of their co…

astro-ph.SR2024

SZ Lyncis: A Non-Accreting Neutron Star-delta Scuti Binary Candidate Discovered via Dynamics and Asteroseismology

Ping Li, Li-Ying Zhu, Wen-Ping Liao

Neutron stars (NSs) are traditionally discovered through radio, X-ray, or gamma-ray observations, but optical time-domain surveys can unveil non-accreting NSs in wide binaries. Her…

astro-ph.SR2024

Evidence for a close-in tertiary orbiting around the Algol-type system HZ Dra with tidal splitting and spots activities

Ping Li, Wen-Ping Liao, Sheng-Bang Qian +7

We reported a cyclic variation of diagram with a semi-amplitude of 0.0033 days and a period of 1.05 years for the pulsating eclipsing binary HZ Dra. The cyclic variation can…

astro-ph.SR2024★ 1 cited

Exploring the physical properties of the Dor binary star RX Dra with photometry and asteroseismology

Li Ping, Liao Wen-Ping, Sun Qi-Bin +1

We model the TESS light curve of the binary system RX Dra, and also first calculate a lot of theoretical models to fit the g-mode frequencies previously detected from the TESS seri…

astro-ph.EP2024★ 7 cited

Using Asteroseismology to Calibrate the Physical Parameters of Confirmed Exoplanets and Their Evolved Host Stars

Wen-Xu Lin, Sheng-Bang Qian, Li-Ying Zhu +2

Asteroseismology offers a profound window into stellar interiors and has emerged as a pivotal technique in exoplanetary research. This study harnesses the Transiting Exoplanet Surv…

astro-ph.SR2024★ 2 cited

KIC 7914906: An Eclipsing Heartbeat Star with Tidally Excited Oscillations and Gamma Doradus/Delta Scuti Hybrid Pulsations

Min-Yu Li, Sheng-Bang Qian, Li-Ying Zhu +6

We present the eclipsing Heartbeat Star KIC 9704906 with tidally excited oscillations (TEOs) and gamma Doradus/delta Scuti hybrid pulsations. The derived parameters show that it ha…

astro-ph.SR2024★ 3 cited

Photometric and Spectroscopic Analysis of V583 Lyrae, an Algol with a g-mode Pulsating Primary and Accretion Disk

Hui-Ting Zhang, Sheng-Bang Qian, Wen-Ping Liao +2

V583 Lyr is an extremely low mass ratio Algol-type binary with an orbital period of 11.2580 days. We determined an effective temperature of T_{eff1} = 9000 \pm 350 K from newly obs…

astro-ph.SR2024

Pulsation Phases and Mode Identification of Tidally Excited Oscillations in Fourteen Kepler Heartbeat Stars

Min-Yu Li, Sheng-Bang Qian, Li-Ying Zhu +6

Tidally excited oscillations (TEOs) in Heartbeat Stars (HBSs) are an essential probe of the internal properties of the systems, but their potential has yet to be fully exploited. B…

astro-ph.SR2024★ 7 cited

A New Window for Studying Intermediate Polars and Tilted Accretion Disk Precession

Qi-Bin Sun, Sheng-Bang Qian, Li-Ying Zhu +5

TV Col is a long-period eclipsing intermediate polar (IPs) prototype star for the negative superhump (NSH) system. We investigate the eclipse minima, eclipse depth, and NSH amplitu…