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M. Palla

13 papers hereh-index 27 citations13 works total

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

author position
  • first author2
  • middle author10
  • last author1

Across the 13 of 13 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA8
  • astro-ph.SR3
  • astro-ph.IM2
same name
  • M. Palla — 31 papers, h 10
  • M. Palla — 1 paper, h 1
  • M. Palla — 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 citedEuropium, we have a problem. Modelling r-process enrichment across Local Group galaxies

8 citations · 19 across the 13 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2026

The oldest low-α thin disc stars

Riano E. Giribaldi, Laura Magrini, Marco Palla +1

The formation pathway of the α-poor Milky Way thin disc remains under debate. The latest observational data indicates the presence of comparable numbers of old stars in both the…

astro-ph.SR2026

The nucleosynthesis of Ba in the Early Universe. Constraints from elemental abundances and isotopic ratios

Riano E. Giribaldi, Marco Palla, Laura Magrini +6

The [Ba/Eu] abundance ratio is commonly adopted as a tracer of the relative contributions of the slow (s) and rapid (r) neutron-capture processes. However, at [Fe/H] < -2 dex, Ba c…

astro-ph.SR2025★ 2 cited

The chemical DNA of the Magellanic Clouds V. R-process dominates neutron capture elements production in the oldest SMC stars

Lorenzo Santarelli, Marco Palla, Alessio Mucciarelli +4

We present the chemical abundances of Fe, alpha- and neutron-capture elements in 12 metal-poor Small Magellanic Cloud (SMC) giant stars, observed with the high-resolution spectrogr…

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