◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

M. de Bennassuti

3 papers here

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

author position
  • first author2
  • middle author1

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

fields
  • astro-ph.GA3

identity via Semantic Scholar / OpenAlex

activity
20142016
most citedLimits on Pop III star formation with the most iron-poor stars

108 citations · 248 across the 3 of their papers we have counts for

collaborators

3 papers

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.GA2014★ 100 cited

Decoding the stellar fossils of the dusty Milky Way progenitors

Matteo de Bennassuti, Raffaella Schneider, Rosa Valiante +1

We investigate the metallicity distribution function (MDF) in the Galactic halo and the relative fraction of Carbon-normal and Carbon-rich stars. To this aim, we use an improved ve…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.