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researcher

Zhen Guo

7 papers hereh-index 429 citations5 works total

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

author position
  • middle author5
  • last author1

Across the 6 of 7 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR5
  • astro-ph.EP1
  • astro-ph.HE1
same name
  • Zhen Guo — 18 papers, h 5
  • Zhen Guo — 12 papers, h 7
  • Zhen Guo — 11 papers, h 9
  • Zhen Guo — 8 papers, h 4
  • Zhen Guo — 7 papers, h 6
  • Zhen Guo — 6 papers, h 4

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

activity
20232026
most citedEvidence of a Disk-wind Origin for Fluorescent H2​ in Classical T Tauri Stars

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

collaborators
Showing 2024Show all

3 papers · 1 filter

astro-ph.SR2024

A Multi-wavelength, Multi-epoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. III. Optical Spectra

John Wendeborn, Catherine C. Espaillat, Thanawuth Thanathibodee +20

Classical T Tauri Stars (CTTSs) are highly variable stars that possess gas- and dust-rich disks from which planets form. Much of their variability is driven by mass accretion from…

astro-ph.SR2024

A Multi-wavelength, Multi-epoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. II. Photometric Light Curves

John Wendeborn, Catherine C. Espaillat, Thanawuth Thanathibodee +8

Classical T Tauri Stars (CTTSs) are young, low-mass stars which accrete material from their surrounding protoplanetary disk. To better understand accretion variability, we conducte…

astro-ph.SR2024★ 1 cited

A Multi-wavelength, Multi-epoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. I. HST FUV and NUV Spectra

John Wendeborn, Catherine C. Espaillat, Sophia Lopez +17

The Classical T Tauri Star (CTTS) stage is a critical phase of the star and planet formation process. In an effort to better understand the mass accretion process, which can dictat…

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