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researcher

G. Cescutti

79 papers hereh-index 262k citations97 works total

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

author position
  • sole author3
  • first author15
  • middle author43
  • last author10

Across the 71 of 79 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA49
  • astro-ph.SR18
  • astro-ph8
  • astro-ph.HE3
  • astro-ph.IM1
same name
  • G. Cescutti — 23 papers, h 9
  • G. Cescutti — 15 papers, h 7
  • G. Cescutti — 13 papers, h 4
  • G. Cescutti — 4 papers
  • G. Cescutti — 2 papers, h 1

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
20052026
most citedChromium: NLTE abundances in metal-poor stars and nucleosynthesis in the Galaxy

188 citations · 2.8k across the 79 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.SR2013★ 142 cited

Solar abundance of manganese: a case for the existence of near Chandrasekhar-mass Type Ia supernova progenitors

Ivo R. Seitenzahl, Gabriele Cescutti, Friedrich K. Roepke +2

Context: Manganese is predominantly synthesised in Type Ia supernova (SN Ia) explosions. Owing to the entropy dependence of the Mn yield in explosive thermonuclear burning, SNe Ia…

astro-ph.GA2013★ 122 cited

The s-process in the Galactic halo: the fifth signature of spinstars in the early Universe?

Gabriele Cescutti, Cristina Chiappini, Raphael Hirschi +2

Very old halo stars were previously found to show at least four different abundance 'anomalies', which models of fast rotating massive stars (spinstars) can successfully account fo…

astro-ph.GA2013

Galactic chemical evolution: The role of the first stars

Gabriele Cescutti, Cristina Chiappini

The massive First Stars (the first ones to contribute to the chemical enrichment of the Universe due to their short lifetimes) are long dead, and even though efforts to directly ob…

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