most citedUnderstanding the origin of CEMP-no stars through ultra-faint dwarfs

20 citations · 48 across the 5 of their papers we have counts for

collaborators

5 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.GA20233 cited

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.…

astro-ph.GA20235 cited

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…

astro-ph.GA202320 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.GA202320 cited

PISN-explorer: hunting the descendants of very massive first stars

D. S. Aguado, S. Salvadori, A. Skúladóttir +6

The very massive first stars () were fundamental to the early phases of reionization, metal enrichment, and super-massive black hole formation. Among them, thos…