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Prominence detection and chromosphere feature on the prototype RS CVn of active binary systems
Dongtao Cao, Shenghong Gu, U Wolter, M Mittag, J H M M Schmitt, Dongyang Gao and Shaoming Hu Monthly Notices of the Royal Astronomical Society 523(3) 4146 (2023) https://doi.org/10.1093/mnras/stad1700
An investigation of the magnetic activity of HD 134319 based on TESS photometry and ground-based spectroscopy
Fukun Xu, Shenghong Gu and Panogiotis Ioannidis Monthly Notices of the Royal Astronomical Society 514(2) 2958 (2022) https://doi.org/10.1093/mnras/stac1233
Physical Properties of Radio Stars Based on LAMOST Spectral Survey
Liyun Zhang, Yao Cheng, Xianming L. Han, Qingfeng Pi, Prabhakar Misra, Baoda Li and Zhongzhong Zhu Universe 8(7) 384 (2022) https://doi.org/10.3390/universe8070384
Magnetic activities on two single-lined RS Canum Venaticorum binaries IM Pegasi and σ Geminorum
Dongtao Cao, Shenghong Gu, F Grundahl and P L Pallé Monthly Notices of the Royal Astronomical Society 514(3) 4190 (2022) https://doi.org/10.1093/mnras/stac1576
Ultraviolet Spectral Behavior of UX Ari with Periodic Flaring Activity
Magnetic Activity and Orbital Period Study for the Short-period RS CVn–type Eclipsing Binary DV Psc
Qing-feng Pi, Li-yun Zhang, Shao-lan Bi, Xianming L. Han, Hong-peng Lu, Qiang Yue, Liu Long and Yan Yan The Astrophysical Journal 877(2) 75 (2019) https://doi.org/10.3847/1538-4357/ab19c3
Prominence activation, optical flare, and post-flare loops on the RS Canum Venaticorum star SZ Piscium
Dongtao Cao, Shenghong Gu, Jian Ge, et al. Monthly Notices of the Royal Astronomical Society 482(1) 988 (2019) https://doi.org/10.1093/mnras/sty2768
Optical flare events on the RS Canum Venaticorum star UX Arietis
Chromospheric activity on late-type star DM UMa using high-resolution spectroscopic observations
LiYun Zhang, QingFeng Pi, Xianming L. Han, Liang Chang and Daimei Wang Monthly Notices of the Royal Astronomical Society 459(1) 854 (2016) https://doi.org/10.1093/mnras/stw668
Chromospheric activity on the late-type star V1355 Ori using Lijiang 1.8-m and 2.4-m telescopes
The new RS CVn binary V1034 Her revisited and the orbital period — activity relation of short-period RS CVn binaries using photometric distortion amplitude