20 citations · 28 across the 3 of their papers we have counts for
3 papers
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…
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…