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researcher

C. Charbonnel

105 papers hereh-index 499k citations303 works total

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

author position
  • sole author2
  • first author12
  • middle author58
  • last author20

Across the 92 of 105 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR43
  • astro-ph40
  • astro-ph.GA14
  • astro-ph.EP8
same name
  • C. Charbonnel — 42 papers, h 19
  • C. Charbonnel — 10 papers, h 7
  • C. Charbonnel — 8 papers, h 4
  • C. Charbonnel — 7 papers, h 4
  • C. Charbonnel — 2 papers
  • C. Charbonnel — 2 papers, h 0

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
19952023
most citedGrids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014)

1.7k citations · 9.5k across the 105 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.GA2023★ 100 cited

Extreme N-emitters at high-redshift: signatures of supermassive stars and globular cluster or black hole formation in action?

R. Marques-Chaves, D. Schaerer, A. Kuruvanthodi +9

[Abridged] Using the JWST/NIRSpec observations from CEERS we found an extreme N-emitter, CEERS-1019 at z=8.6782 showing intense NIV and NIII emission. From the observed rest-UV and…

astro-ph.GA2023★ 105 cited

N-enhancement in GN-z11: First evidence for supermassive stars nucleosynthesis in proto-globular clusters-like conditions at high redshift ?

C. Charbonnel, D. Schaerer, N. Prantzos +5

Unusually high N/O abundance ratios were recently reported for a very compact, intensively star-forming object GN-z11 at z=10.6 from JWST/NIRSpec observations. We present an empi…

astro-ph.GA2023★ 3 cited

Search strategies for supermassive stars in young clusters and application to nearby galaxies

A. Kuruvanthodi, D. Schaerer, M. Messa +4

Supermassive stars (SMS) with masses M≳103−104M⊙​, formed by runaway collisions in young, massive, and dense star clusters have been invoked as a possible soluti…

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