97 citations · 233 across the 5 of their papers we have counts for
7 papers
The effects of different Type Ia SN yields on Milky Way chemical evolution
Marco Palla
We study the effect of different Type Ia SN nucleosynthesis prescriptions on the Milky Way chemical evolution. To this aim, we run detailed one-infall and two-infall chemical evolu…
APOGEE DR16: a multi-zone chemical evolution model for the Galactic disc based on MCMC methods
E. Spitoni, K. Verma, V. Silva Aguirre +6
The analysis of the APOGEE DR16 data suggests the existence of a clear distinction between two sequences of disc stars at different Galactocentric distances in the [/Fe] vs. [Fe…
Chemical evolution of the Milky Way: constraints on the formation of the thick and thin discs
Marco Palla, Francesca Matteucci, Emanuele Spitoni +2
We study the evolution of Milky Way thick and thin discs in the light of the most recent observational data. In particular, we analyze abundance gradients of O, N, Fe and Mg along…
Galactic archaeology at high redshift: inferring the nature of GRB host galaxies from abundances
Marco Palla, Francesca Matteucci, Francesco Calura +1
We identify the nature of high redshift long Gamma-Ray Bursts (LGRBs) host galaxies by comparing the observed abundance ratios in the interstellar medium with detailed chemical evo…
The influence of a top-heavy integrated galactic IMF and dust on the chemical evolution of high-redshift starbursts
Marco Palla, Francesco Calura, Francesca Matteucci +3
We study the effects of the integrated galactic initial mass function (IGIMF) and dust evolution on the abundance patterns of high redshift starburst galaxies. In our chemical mode…
On the Origin of Dust in Galaxy Clusters at Low to Intermediate Redshift
Eda Gjergo, Francesca Matteucci, Marco Palla +3
Stacked analyses of galaxy clusters at low-to-intermediate redshift show signatures attributable to dust, but the origin of this dust is uncertain. We test the hypothesis that the…