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most citedCSS_J154915.7+375506: A low-mass-ratio marginal contact binary system with a hierarchical third body

5 citations · 14 across the 8 of their papers we have counts for

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7 papers · 1 filter

astro-ph.SR2026★ 1 cited

Diversity in Evolutionary Status and Magnetic Activity among Solar-Type Twin Detached Eclipsing Binaries

Fang-Bin Meng, Li-Ying Zhu, Sheng-Bang Qian +9

We present a combined photometric and spectroscopic analysis of four detached eclipsing binaries (KIC 8957954, KIC 10593759, KIC 8302455, and TIC 207398432), all of which exhibit c…

astro-ph.SR2026

HD 26172: an active solar-type subgiant in a close binary system

Fang-Bin Meng, Li-Ying Zhu, Sheng-Bang Qian +5

We present the first comprehensive photometric and spectroscopic analysis of the RS CVn system HD 26172, robustly determining the previously debated evolutionary state of its prima…

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.SR2024★ 5 cited

KM UMa: An active short-period detached eclipsing binary in a hierarchical quadruple system

Fangbin Meng, Liying Zhu, Nianping Liu +4

The first detailed photometric and spectroscopic analysis of the G-type eclipsing binary KM UMa is presented, which indicates that the system is a short-period detached eclipsing b…

astro-ph.SR2024

Deep and low mass-ratio contact binaries and their third bodies

Liying Zhu, Shengbang Qian, Wenping Liao +6

Deep and low mass-ratio contact binaries (DLMCBs) are believed to be in the final stage of their contact phase, potentially leading to the formation of fast-rotating single stars s…

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…