activity
20142017
most citedLimits on Pop III star formation with the most iron-poor stars

108 citations · 332 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2017★ 46 cited

The formation and coalescence sites of the first gravitational wave events

Raffaella Schneider, Luca Graziani, Stefania Marassi +4

We present a novel theoretical model to characterize the formation and coalescence sites of compact binaries in a cosmological context. This is based on the coupling between the bi…

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 to . 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.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…