activity
20242026
most citedFurther Investigation on Chromospheric Activity Patterns of the RS Canum Venaticorum Star V711 Tauri

3 citations · 6 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.SR20262 cited

Doppler-shifted Signatures in the Chromospheric Line Profiles of II Pegasi

Cao Dongtao, Gu shenghong

Stellar flares are frequently accompanied by prominence eruptions, coronal mass ejections (CMEs), and other forms of plasma motion. Based on the long-term high-resolution spectrosc…

astro-ph.SR20263 cited

Further Investigation on Chromospheric Activity Patterns of the RS Canum Venaticorum Star V711 Tauri

Cao Dongtao, Gu Shenghong

We present new long-term spectroscopic observations of the very active RS Canum Venaticorum (RS CVn) star V711 Tauri (V711 Tau), obtained during several observing runs from 2005 to…

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.SR20261 cited

Investigating Possible Stellar Coronal Mass Ejections in M-type Dwarfs Using the CARMENES DR1 Spectra

Cao Dongtao, Gu Shenghong

Stellar coronal mass ejections (CMEs) have significant impacts on surrounding exoplanets and stellar evolution. For M-type dwarf stars, hosting close-in habitable zones, frequent a…

astro-ph.SR2025

Magnetic activity of ultracool dwarfs in the LAMOST DR11

Yue Xiang, Shenghong Gu, Dongtao Cao

Ultracool dwarfs consist of lowest-mass stars and brown dwarfs. Their interior is fully convective, different from that of the partly-convective Sun-like stars. Magnetic field gene…

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…