activity
20182024
most citedZero-metallicity hypernova uncovered by an ultra metal-poor star in the Sculptor dwarf spheroidal galaxy

62 citations · 197 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.GA202162 cited

Zero-metallicity hypernova uncovered by an ultra metal-poor star in the Sculptor dwarf spheroidal galaxy

Ása Skúladóttir, Stefania Salvadori, Anish M. Amarsi +9

Although true metal-free "Population III" stars have so-far escaped discovery, their nature, and that of their supernovae, is revealed in the chemical products left behind in the n…

astro-ph.GA202154 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…

astro-ph.GA2020

Neutron-capture elements in dwarf galaxies III: A homogenized analysis of 13 dwarf spheroidal and ultra-faint galaxies

Moritz Reichert, Camilla J. Hansen, Michael Hanke +3

We present a large homogeneous set of stellar parameters and abundances across a broad range of metallicities, involving classical dwarf spheroidal (dSph) and ultra-faint dSph…

astro-ph.GA201920 cited

Neutron-capture elements in dwarf galaxies I: Chemical clocks & the short timescale of the r-process

Ása Skúladóttir, Camilla Juul Hansen, Stefania Salvadori +1

The heavy elements (Z>30) are created in neutron-capture processes which happen at very different nucleosynthetic sites. To study them in an environment different from the Milky Wa…

astro-ph.GA201961 cited

Probing the existence of very massive first stars

S. Salvadori, P. Bonifacio, E. Caffau +4

We present a novel approach aimed at identifying the key chemical elements to search for the (missing) descendants of very massive first stars exploding as Pair Instability Superno…

astro-ph.GA2019

4MOST Consortium Survey 2: The Milky Way Halo High-Resolution Survey

N. Christlieb, C. Battistini, P. Bonifacio +19

We will study the formation history of the Milky Way, and the earliest phases of its chemical enrichment, with a sample of more than 1.5 million stars at high galactic latitude. El…