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researcher

C. Chen

61 papers hereh-index 261.7k citations80 works total

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

author position
  • first author5
  • middle author42
  • last author8

Across the 55 of 61 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA34
  • astro-ph11
  • astro-ph.SR8
  • astro-ph.CO3
  • astro-ph.HE3
  • astro-ph.EP2
same name
  • C. Chen — 470 papers
  • C. Chen — 206 papers, h 93
  • C. Chen — 184 papers, h 5
  • C. Chen — 173 papers, h 20
  • C. Chen — 170 papers, h 6
  • C. Chen — 154 papers, h 20

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
19992026
most citedSurveying the Agents of Galaxy Evolution in the Tidally-Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC). I. Overview

225 citations · 2k across the 61 of their papers we have counts for

collaborators
Showing 2025 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2025★ 5 cited

Protostars at Subsolar Metallicity: First Detection of Large Solid-state Complex Organic Molecules in the Large Magellanic Cloud

Marta Sewiło, Will R. M. Rocha, Martijn van Gelder +11

We present the results of James Webb Space Telescope observations of the protostar ST6 in the Large Magellanic Cloud (LMC) with the Medium Resolution Spectrograph of the Mid-Infrar…

astro-ph.GA2025

Oxygen isotopes reveal low-mass star dominance in the Small Magellanic Cloud

Yan Gong, Zhi-yu Zhang, Christian Henkel +9

Oxygen isotope abundances and their ratios are fingerprints of stellar evolution and therefore provide a powerful tool in tracing the enrichment history of galaxies. However, their…

astro-ph.GA2025

LMC+: Large-scale mapping of [CII] and [OIII] in the LMC molecular ridge, I. Dataset and line ratio analyses

C. Fischer, S. C. Madden, A. Krabbe +29

The fundamental process of star formation in galaxies involves the interplay between the fueling of star formation via molecular gas and the feedback from recently formed massive s…

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