47 citations · 117 across the 6 of their papers we have counts for
7 papers
Chemical evolution of the inner 2 degrees of the Milky Way bulge: [alpha/Fe] trends and metallicity gradients
N. Ryde, M. Schultheis, V. Grieco +3
The structure, formation, and evolution of the Milky Way bulge is a matter of debate. Important diagnostics for discriminating between bulge models include alpha-abundance trends w…
Chemical evolution of the Galactic Center
V. Grieco, F. Matteucci, N. Ryde +2
In recent years, the Galactic Center (GC) region (200 pc in radius) has been studied in detail with spectroscopic stellar data as well as an estimate of the ongoing star formation…
Chemical evolution of the bulge of M31: predictions about abundance ratios
M. M. Marcon-Uchida, F. Matteucci, G. A. Lanfranchi +2
We aim at reproducing the chemical evolution of the bulge of M31 by means of a detailed chemical evolution model, including radial gas flows coming from the disk. We study the impa…
Chemical evolution models: GRB host identification and cosmic dust predictions
V. Grieco, F. Matteucci, F. Calura +3
The nature of some GRB host galaxies has been investigated by means of chemical evolution models of galaxies of different morphological type following the evolution of the abundanc…
Galactic and Cosmic Type Ia SN rates: is it possible to impose constraints on SNIa progenitors?
I. Bonaparte, F. Matteucci, S. Recchi +3
We compute the Type Ia supernova rates in typical elliptical galaxies by varying the progenitor models for Type Ia supernovae. To do that a formalism which takes into account the d…
Chemical evolution of the Galactic bulge: different stellar populations and possible gradients
V. Grieco, F. Matteucci, A. Pipino +1
We compute the chemical evolution of the Galactic bulge to explain the existence of two main stellar populations recently observed. After comparing model results and observational…