85 citations · 192 across the 4 of their papers we have counts for
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About the Chemical Evolution of dSphs (and the peculiar Globular Cluster Omega Cen)
Andrea Marcolini, Annibale D'Ercole
We present three dimensional hydrodynamical simulations aimed at studying the dynamical and chemical evolution of the interstellar medium (ISM) in isolated dwarf spheroidal galaxie…
The Chemical Evolution of Dwarf Spheroidal Galaxies: Dissecting the Inner Regions and their Stellar Populations
A. Marcolini, A. D'Ercole, G. Battaglia +1
Using 3-dimensional hydrodynamical simulations of isolated dwarf spheroidal galaxies (dSphs), we undertake an analysis of the chemical properties of their inner regions, identifyin…
Modeling the chemical evolution of Omega Centauri using three-dimensional hydrodynamical simulations
A. Marcolini, A. Sollima, A. D'Ercole +2
We present a hydrodynamical and chemical model for the globular cluster Omega Cen, under the assumption that it is the remnant of an ancient dwarf spheroidal galaxy (dSph), the bul…
Star formation feedback and metal enrichment by SN Ia and SN II in dwarf spheroidal galaxies: the case of Draco
A. Marcolini, A. D'Ercole, F. Brighenti +1
We present 3D hydrodynamical simulations aimed to study the dynamical and chemical evolution of the interstellar medium in dwarf spheroidal galaxies. This evolution is driven by th…
Active Galactic Nuclei in the mid-IR. Evolution and Contribution to the Cosmic Infrared Background
I. Matute, F. La Franca, F. Pozzi +3
We study the evolution of the luminosity function (LF) of type-1 and type-2 AGN in the mid-infrared, and derive their contribution to the Cosmic InfraRed Background (CIRB) and the…
The dynamics and high-energy emission of conductive gas clouds in supernova-driven galactic superwinds
A. Marcolini, D. K. Strickland, A. D'Ercole +2
In this paper we present high-resolution hydrodynamical models of warm ionized clouds embedded in a superwind, and compare the OVI and soft X-ray properties to the existing observa…