activity
20222026
most citedPossible detection of coronal mass ejections on late-type main-sequence stars in LAMOST medium-resolution spectra

44 citations · 108 across the 15 of their papers we have counts for

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13 papers · 1 filter

astro-ph.SR2026★ 2 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.SR2026★ 3 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.SR2026★ 1 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.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.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…

astro-ph.SR2024★ 15 cited

Red Asymmetry of H Line Profiles during the flares on the active RS CVn-type star II Pegasi

Dongtao Cao, Shenghong Gu

Stellar coronal mass ejections (CMEs) have recently attracted much attention for their impacts on stellar evolution and surrounding exoplanets. RS CVn-type stars could produce larg…

astro-ph.SR2024★ 20 cited

Prominence activation, optical flare, and post-flare loops on the RS Canum Venaticorum star SZ Piscium

Dongtao Cao, Shenghong Gu, Jian Ge +7

We present the results of time-resolved high-resolution spectroscopic observations of the very active RS Canum Venaticorum (RS CVn) star SZ Piscium (SZ Psc), obtained during two co…

astro-ph.SR2024★ 4 cited

Magnetic activities on two single-lined RS Canum Venaticorum binaries IM Pegasi and Geminorum

Dongtao Cao, Shenghong Gu, F. Grundahl +1

We present the study on continuous high-resolution spectroscopic observations of two long-period single-lined RS Canum Venaticorum (RS CVn) binary stars IM Pegasi (IM Peg) and …

astro-ph.SR2024★ 7 cited

Prominence detection and chromosphere feature on the prototype RS CVn of active binary systems

Dongtao Cao, Shenghong Gu, U. Wolter +4

We present a study of high-resolution spectra of RS Canum Venaticorum (RS CVn), a prototype of active binary systems. Our data were obtained from 1998 to 2017 using different teles…

astro-ph.SR2022★ 7 cited

Investigation of stellar magnetic activity using variational autoencoder based on low-resolution spectroscopic survey

Yue Xiang, Shenghong Gu, Dongtao Cao

We apply the variational autoencoder (VAE) to the LAMOST-K2 low-resolution spectra to detect the magnetic activity of the stars in the K2 field. After the training on the spectra o…

astro-ph.SR2022★ 44 cited

Possible detection of coronal mass ejections on late-type main-sequence stars in LAMOST medium-resolution spectra

Hong-peng Lu, Hui Tian, Li-yun Zhang +9

Context. Stellar coronal mass ejections (CMEs) are the primary driver of the exoplanetary space weather and they could affect the habitability of exoplanets. However, detections of…