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researcher

C. Charbonnel

8 papers hereh-index 4207 citations10 works total

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

author position
  • middle author5

Across the 5 of 8 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA5
  • astro-ph.SR3
same name
  • C. Charbonnel — 105 papers, h 49
  • C. Charbonnel — 42 papers, h 19
  • C. Charbonnel — 10 papers, h 7
  • 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
20202026
most citedStar clusters near and far; tracing star formation across cosmic time

136 citations · 408 across the 8 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2026

A quasi-star is born: formation and evolution of accreting quasi-stars as a pathway to Little Red Dots at non-zero metallicity

J. Roman-Garza, C. Charbonnel, D. Schaerer +5

The recently discovered Little Red Dots identified by the James Webb Space Telescope are compact high-redshift sources whose properties have motivated models involving black holes…

astro-ph.SR2026★ 1 cited

Massive stellar cannibals: How stellar mergers drive mass-loss in extremely massive stars

J. Roman-Garza, T. Fragos, C. Charbonnel +3

It has been theorized that the formation of extremely massive and supermassive stars (>103 M⊙​) could plausibly be the outcome of stellar mergers in low metallicity (…

astro-ph.SR2025★ 9 cited

Collision-induced mass loss and mass gain on an extremely massive star. An analytical approach and a static proto-globular cluster test-case

Laura Ramírez-Galeano, Corinne Charbonnel, Tassos Fragos +3

The objective of this study is to analytically explore mass loss and gain induced by stellar collisions on a gas-accreting extremely massive star (aEMS, 10^3 <= M/M_sun <= 10^4). W…

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