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20162026
most citedNew pulsating stars detected in EA-type eclipsing binary systems based on TESS data

42 citations · 129 across the 15 of their papers we have counts for

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7 papers · 1 filter

astro-ph.SR2024★ 5 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…

astro-ph.SR2024★ 7 cited

A catalog of new slowly pulsating B-type stars

Xiang-dong Shi, Sheng-bang Qian, Li-ying Zhu +1

This paper reports the discovery of new slowly pulsating B-type stars. Based on the photometric, spectral, and astrometric data of TESS, LAMOST, and Gaia surveys, we have found 286…

astro-ph.SR2024★ 42 cited

New pulsating stars detected in EA-type eclipsing binary systems based on TESS data

Xiang-Dong Shi, Sheng-Bang Qian, Lin-Jia Li

Pulsating stars in eclipsing binaries are very important to understand stellar interior structures through astroseismology because their absolute parameters such as the masses and…

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

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★ 5 cited

CSS_J154915.7+375506: A low-mass-ratio marginal contact binary system with a hierarchical third body

Jin-Feng Wu, Li-Ying Zhu, Azizbek Matekov +6

We presented the multi-filter light curves of CSS_J154915.7+375506 inaugurally, which were observed by the 1.5 m AZT-22 telescope at Maidanak Astronomical Observatory. A low-resolu…