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M. Rossi

4 papers here

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

author position
  • first author1
  • middle author3

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

fields
  • astro-ph.GA4
ORCID 0000-0001-6887-2663
same name
  • M. Rossi — 19 papers, h 30
  • M. Rossi — 18 papers
  • M. Rossi — 18 papers, h 11
  • M. Rossi — 16 papers, h 20
  • M. Rossi — 16 papers, h 19
  • M. Rossi — 16 papers, h 23

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 citedThe energy distribution of the first supernovae

24 citations · 58 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2023

Characterising the true descendants of the first stars

Irene Vanni, Stefania Salvadori, Ása Skúladóttir +2

The metal-poor stars in the Galactic halo are thought to show the imprints of the first (PopIII) stars, and thus provide a glance at the first episodes of star formation. In this w…

astro-ph.GA2023★ 24 cited

The energy distribution of the first supernovae

I. Koutsouridou, S. Salvadori, Á. Skúladóttir +3

The nature of the first Pop III stars is still a mystery and the energy distribution of the first supernovae is completely unexplored. For the first time we account simultaneously…

astro-ph.GA2023★ 14 cited

On the dearth of C-enhanced metal-poor stars in the Galactic bulge

Giulia Pagnini, Stefania Salvadori, Martina Rossi +3

The chemical fingerprints of the first stars are retained within the photospheres of ancient unevolved metal-poor stars. A significant fraction of these stellar fossils is represen…

astro-ph.GA2023★ 20 cited

Understanding the origin of CEMP-no stars through ultra-faint dwarfs

Martina Rossi, Stefania Salvadori, Ása Skúladóttir +1

The origin of Carbon Enhanced Metal-Poor (CEMP-no) stars with low abundances of neutron-capture elements is still unclear. These stars are ubiquitous, found primarily in the Milky…

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