activity
20002004
most citedClassical Limit of Quantum Dynamical Entropies

13 citations · 13 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph2004

Chemical Evolution of Late-type Dwarf Galaxies - The windy starburst dwarfs NGC 1569 and NGC 1705

Donatella Romano, Monica Tosi, Francesca Matteucci

Thanks to the capabilities of modern telescopes and instrumentation, it is now possible to resolve single stars in external dwarf galaxies, provided they are bright enough. For gal…

astro-ph2004

Quantifying the uncertainties of chemical evolution studies. I. The stellar initial mass function and the stellar lifetimes

Donatella Romano, Cristina Chiappini, Francesca Matteucci +1

The stellar initial mass function and the stellar lifetimes are basic ingredients of chemical evolution models, for which different recipes can be found in the literature. In this…

quant-ph200313 cited

Classical Limit of Quantum Dynamical Entropies

F. Benatti, V. Cappellini, M. De Cock +2

Two non-commutative dynamical entropies are studied in connection with the classical limit. For systems with a strongly chaotic classical limit, the Kolmogorov-Sinai invariant is r…

astro-ph2001

Chemical Evolution of Elliptical Galaxies as a Constraint to Galaxy Formation Scenarios

Donatella Romano, Francesca Matteucci, Luigi Danese

Elliptical galaxies are the main contributors to the chemical enrichment of the intracluster and intergalactic medium; understanding how they form and evolve enables us to get impo…

astro-ph2000

Chemical and dynamical evolution in gas-rich dwarf galaxies

Simone Recchi, Francesca Matteucci, Annibale D'Ercole

We study the effect of a single, instantaneous starburst in a gas-rich dwarf galaxy on the dynamical and chemical evolution of its interstellar medium. We consider the energetic in…

astro-ph1998

Light and Heavy Elements in the Galactic Bulge

F. Matteucci, D. Romano, P. Molaro

The chemical evolution of the Galactic bulge is treated here in the context of an inside-out model for the Galaxy formation. We assume that this central region evolved even faster…