activity
20232026
most citedFirst discovery of QPOs in the dwarf nova HS 2325+8205 based on TESS photometry

17 citations · 100 across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph.SR2026

Eclipse Properties and Superhump Evolution in the SU UMa-Type Dwarf Nova Z Cha

Qi-Bin Sun, Sheng-Bang Qian, Li-Ying Zhu +10

The advent of large-scale time-domain surveys provides both opportunities and challenges for understanding accretion disk evolution in cataclysmic variables (CVs). Using high-caden…

astro-ph.HE2026

Universal scaling between magnetar field and initial spin period for short gamma ray bursts

Qin-Mei Li, Qi-Bin Sun, Sheng-Bang Qian +5

The -- correlation serves as a critical probe of magnetar engine physics. Although this scaling relation has been firmly established for long gamma-ray bursts (lGRBs), sy…

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

Asteroseismology and Dynamics Reveal Interior Structure and Coeval Evolution in the Triply Post-Main-Sequence system DG Leo

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

Scuti stars in binary or multiple systems serve as crucial probes for studying stellar pulsation and evolution. However, many such systems are not ideal for asteroseismology du…

astro-ph.HE2025

New Evidence for Extragalactic Einstein Probe Transients associated with Long Gamma-ray Bursts

Qin-Mei Li, Qi-Bin Sun, Sheng-Bang Qian +1

The origin of extragalactic fast X-ray transients (EFXTs) remains a fundamental open question in high-energy astrophysics. The Einstein Probe (EP) mission provides a transformative…

astro-ph.HE2025

The Cosmic Star Formation History: Insights from Kilonova-Associated Gamma-Ray Bursts

Qin-Mei Li, Qi-Bin Sun, Sheng-Bang Qian +2

The origin of the Universe and its material content remains one of the most fundamental questions in science. Gamma-ray bursts (GRBs), with their extreme luminosities and high-reds…

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.HE2025★ 2 cited

Detection of Low-Redshift Excess in Supernova-Linked Gamma-Ray Bursts

Qin-Mei Li, Qi-Bin Sun, Sheng-Bang Qian +1

Gamma-ray bursts (GRBs) are traditionally classified into long (lGRBs) and short (sGRBs) durations based on their , with lGRBs widely used as tracers of the cosmic star for…

astro-ph.SR2025★ 1 cited

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.SR2024★ 5 cited

Superoutbursts and Positive Superhumps Occurred During the Standstill of a Z Cam-type Dwarf Nova

Qi-Bin Sun, Sheng-Bang Qian, Li-Ying Zhu +4

Dwarf novae are semi-detached binaries, where a white dwarf accretes material from a cool main-sequence companion via an accretion disk, and are known for their intermittent outbur…

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★ 5 cited

A New IW And-Type Star: Karachurin 12 with Tilted Disks and Diverse cycles

Qi-Bin Sun, Sheng-Bang Qian, Li-Ying Zhu +4

The IW And-type phenomenon in cataclysmic variables presents a significant challenge to the accretion disk instability model. Using photometric data from the All-Sky Automated Surv…

astro-ph.SR2024★ 6 cited

Tilted Disk Precession and Negative Superhumps in HS 2325+8205: A Multi-Window Analysis

Qi-Bin Sun, Sheng-Bang Qian, Li-Ying Zhu +3

Tilted disk precession exists in different objects. Negative superhumps (NSHs) in cataclysmic variable stars (CVs) are believed to arise from the interaction between the reverse pr…

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.HE2024★ 4 cited

Comparison of the Origin of Short Gamma-Ray Bursts with or without Extended Emission

Qin-Mei Li, Qi-Bin Sun

The merger of compact binary stars produces short gamma-ray bursts (sGRBs), involving channels such as neutron star - neutron star (BNS) and neutron star - black hole (NS-BH). The…

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.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

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…

astro-ph.SR2023★ 11 cited

Evolution of negative superhumps, quasi-periodic oscillations and outbursts in the Z Cam-type dwarf nova AH Her

Qi-Bin Sun, Sheng-Bang Qian, Min-Yu Li

AH Her is a Z Cam-type dwarf nova with an orbital period of ~ 0.258 d. Dwarf nova oscillations and long-period dwarf nova oscillations have been detected, but no quasi-periodic osc…

astro-ph.SR2023★ 13 cited

Nine New Cataclysmic Variable Stars with Negative Superhumps

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

Negative superhumps (NSHs) are signals a few percent shorter than the orbital period of a binary star and are considered to originate from the reverse precession of the tilted disk…

astro-ph.SR2023★ 8 cited

Detection of Tidally Excited Oscillations in Kepler Heartbeat Stars

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

Heartbeat stars (HBSs) with tidally excited oscillations (TEOs) are ideal laboratories for studying the effect of equilibrium and dynamical tides. However, studies of TEOs in Keple…