105 citations · 352 across the 11 of their papers we have counts for
11 papers
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…
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…
First stars signatures in high-z absorbers
Stefania Salvadori, Valentina D'Odorico, Andrea Saccardi +2
The first stars were likely more massive than those forming today and thus rapidly evolved, exploding as supernovae and enriching the surrounding gas with their chemical products.…
Are all metal-poor stars of second-generation?
Irene Vanni, Stefania Salvadori, Ása Skúladóttir
Hydrodynamical cosmological simulations predict that the metal-free Population III (Pop III) stars were likely very massive and, therefore, short-lived. However, they left their ch…
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…
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…