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

3 citations · 6 across the 4 of their papers we have counts for

collaborators

7 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…

physics.plasm-ph2026

A Hybrid Scheme to Achieve Highest Implosion Performance on the OMEGA Laser

P. S. Farmakis, L. Ceurvorst, V. Gopalaswamy +5

Merging direct and indirect-drive has long been viewed as an optimal hybrid laser-fusion scheme that combines the uniformity of x rays with the efficiency of direct illumination. W…

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…