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S. Gu

4 papers hereh-index 444 citations13 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author1
  • last author3

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
same name
  • S. Gu — 2 papers, h 4
  • S. Gu — 1 paper, h 4
  • S. Gu — 1 paper, h 6
  • S. Gu — 1 paper, h 4
  • S. Gu — 1 paper, h 0
  • S. Gu — 1 paper, h 43

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

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

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

collaborators

4 papers

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★ 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.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…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.