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researcher

M. Pignatari

7 papers hereh-index 14 citations10 works total

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

author position
  • middle author3
  • last author4

Across the 7 of 7 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
  • astro-ph.GA2
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • M. Pignatari — 18 papers, h 42
  • M. Pignatari — 1 paper, h 3

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

works on
chemical evolution 1heavy elements 1open clusters 1s-process nucleosynthesis 1stellar spectroscopy 1

From the 1 of 7 linked papers with an AI index.

most citedProduction of heavy I^±-elements and 44Ti in Cas A: comparison to abundances from 1D core-collapse supernova models and evidence for Carbon-Oxygen shell mergers

2 citations · 2 across the 3 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

2 papers · 1 filter

astro-ph.GA2026

Stellar Population Astrophysics (SPA) with the TNG. Beyond the iron peak: Galactic evolution of molybdenum, ruthenium and zirconium through open clusters

Natalia Alvarez-Baena, Valentina D'Orazi, Christopher Sneden +11

The paper measures molybdenum, ruthenium, and zirconium abundances in 81 stars from 30 open clusters using high‑resolution HARPS‑N spectra to investigate the Galactic chemical evol…

astro-ph.GA2025

Molybdenum and ruthenium in the Galactic disk: A closer look at their nucleosynthesis components

Tamara Mishenina, Teresa Kurtukian-Nieto, Tatiana Gorbaneva +3

The stellar origin of the elements molybdenum (Mo, Z=42) and ruthenium (Ru, Z=44) is still a matter of debate. Studying their abundances provides valuable insights into nucleosynth…

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