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researcher

Stefania Salvadori

4 papers hereh-index 226 citations2 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author2
  • last author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph.CO1
same name
  • Stefania Salvadori — 19 papers, h 5

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20092017
most citedLimits on Pop III star formation with the most iron-poor stars

108 citations · 260 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2017★ 38 cited

The history of the dark and luminous side of Milky Way-like progenitors

Luca Graziani, M. de Bennassuti, R. Schneider +2

Here we investigate the evolution of a Milky Way (MW) -like galaxy with the aim of predicting the properties of its progenitors all the way from z∼20 to z=0. We apply GA…

astro-ph.GA2016★ 108 cited

Limits on Pop III star formation with the most iron-poor stars

M. de Bennassuti, S. Salvadori, R. Schneider +2

We study the impact of star-forming mini-haloes, and the Initial Mass Function (IMF) of Population III (Pop III) stars, on the Galactic halo Metallicity Distribution Function (MDF)…

astro-ph.GA2015★ 40 cited

Galaxy formation with radiative and chemical feedback

L. Graziani, S. Salvadori, R. Schneider +3

Here we introduce GAMESH, a novel pipeline which implements self-consistent radiative and chemical feedback in a computational model of galaxy formation. By combining the cosmologi…

astro-ph.CO2009★ 74 cited

Mining the Galactic Halo for Very Metal-Poor Stars

S. Salvadori, A. Ferrara, R. Schneider +2

We study the age and metallicity distribution function (MDF) of metal-poor stars in the Milky Way halo as a function of galactocentric radius by combining N-body simulations and se…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.