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20242026
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astro-ph.SR2026

A Possible Stellar CME Event Associated with a Long-duration Optical Flare on the RS CVn-type Star UX Arietis

Cao Dongtao, Gu Shenghong

Coronal mass ejections (CMEs) are large-scale eruptions of magnetized plasma from stellar coronae, and they are always accompanied by flares. In this study, we present high-resolut…

astro-ph.SR2026

A Search for Exoplanets around Northern Circumpolar Stars X. The origin of radial velocity variations in the evolved star HD 216595

Sang-Hee Kim, Byeong-Cheol Lee, Shenghong Gu +9

Detecting planetary companions around evolved stars, particularly asymptotic giant branch (AGB) stars, is challenging due to intrinsic stellar variability such as surface convectio…

astro-ph.SR2026

Starspot activity and surface differential rotation on UX Arietis

Yue Xiang, Shenghong Gu, A. Collier Cameron +2

We present new Doppler images of the K0 subgiant primary component of the RS CVn-type binary UX Arietis (UX Ari), derived from time-series spectra obtained in November--December of…

astro-ph.SR2024

Further study of starspot activity and measurement of differential rotation for SZ Piscium

Yue Xiang, Shenghong Gu, A. Collier Cameron +2

We present a series of 9 Doppler images of the magnetically active K component of the RS CVn-type binary SZ Psc, based on the high-resolution spectroscopic data collected from 2014…

astro-ph.SR2024

Stellar cycle and evolution of polar spots in an M+WD binary

Xinlin Zhao, Song Wang, Xue Li +4

Stellar activity cycles reveal continuous relaxation and induction of magnetic fields. The activity cycle is typically traced through the observation of cyclic variations in total…