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

17 citations · 88 across the 23 of their papers we have counts for

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16 papers · 1 filter

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.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★ 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★ 2 cited

Detection of two totally eclipsing B-type binaries with extremely low mass ratios

Linfeng Chang, Shengbang Qian, Lei Zang +1

The detection of O- and B-type stars with extremely low-mass companions is very important for understanding the formation and evolution of binary stars. However, their finding rema…

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

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★ 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★ 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…

astro-ph.SR2023★ 15 cited

New evidence for the precession of tilted disk in SDSS J081256.85+191157.8

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

Super-orbital signals and negative superhumps are thought to be related to the reverse precession of the nodal line in a tilted disk, but the evidence is lacking. Our results provi…

astro-ph.SR2023★ 17 cited

First discovery of QPOs in the dwarf nova HS 2325+8205 based on TESS photometry

Qi-Bin Sun, Sheng-Bang Qian, Li-Ying Zhu +9

HS 2325+8205 is a long-period eclipsing dwarf nova with an orbital period above the period gap (Porb>3 h) and is reported to be a Z Cam-type dwarf nova. Based on the photometry of…