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M. Limongi

4 papers hereh-index 358 citations6 works total

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

author position
  • middle author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR2
  • astro-ph1
  • astro-ph.GA1
same name
  • M. Limongi — 83 papers, h 38
  • M. Limongi — 8 papers, h 3
  • M. Limongi — 1 paper, 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

most citedSynthetic properties of bright metal-poor variables. I. "Anomalous" Cepheids

38 citations · 67 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2025★ 4 cited

Unveiling the nature of HE 0107-5240

E. Caffau, M. Steffen, P. Molaro +27

The vast majority of the most iron-poor stars in the Galaxy exhibit a strong carbon enhancement, with C/H ratios only about two orders of magnitude below solar. This unusual chemic…

astro-ph.SR2025★ 13 cited

The Occurrence and Impact of Carbon-Oxygen Shell Mergers in Massive Stars

L. Roberti, M. Pignatari, H. E. Brinkman +6

In their final stages before undergoing a core-collapse supernova, massive stars may experience mergers between internal shells where carbon (C) and oxygen (O) are consumed as fuel…

astro-ph.GA2025★ 12 cited

Explaining the 12C/13C ratio in the Galactic halo: the contribution from shell mergers in primordial massive stars

F. Rizzuti, G. Cescutti, P. Molaro +5

Recent campaigns of observations have provided new measurements of the carbon isotopes in the most metal-poor stars of the Galaxy. These stars are so metal-poor that they could onl…

astro-ph2006★ 38 cited

Synthetic properties of bright metal-poor variables. I. "Anomalous" Cepheids

G. Fiorentino, M. Limongi, F. Caputo +1

We present new grids of evolutionary models for the so-colled ``Anomalous'' Cepheids (ACs), adopting Z=0.0001 and various assumptions on the progenitor mass and mass-loss efficienc…

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