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20212024
most citedUltra-faint dwarf galaxies: unveiling the minimum mass of the first stars

54 citations · 115 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2024★ 3 cited

Hidden Population III Descendants in Ultra-Faint Dwarf Galaxies

Martina Rossi, Stefania Salvadori, Ása Skúladóttir +2

The elusive properties of the first (Pop III) stars can be indirectly unveiled by uncovering their true descendants. To this aim, we exploit our data-calibrated model for the best-…

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…

astro-ph.GA2021★ 54 cited

Ultra-faint dwarf galaxies: unveiling the minimum mass of the first stars

Martina Rossi, Stefania Salvadori, Ása Skúladóttir

The non-detection of zero-metallicity stars in ultra-faint dwarf galaxies (UFDs) can be used to constrain the Initial Mass Function (IMF) of the first (PopIII) stars by means of a…