activity
20042018
most citedModelling galaxy spectra in presence of interstellar dust. I. The model of ISM and the library of dusty SSPs

51 citations · 325 across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.GA2018★ 16 cited

GalMod: a Galactic synthesis population model

S. Pasetto, E. K. Grebel, C. Chiosi +7

We present a new Galaxy population synthesis Model (GalMod). GalMod is a star-count model featuring an asymmetric bar/bulge as well as spiral arms and related extinction. The model…

astro-ph.GA2014★ 7 cited

Modelling galaxy spectra in presence of interstellar dust-III. From nearby galaxies to the distant Universe

Letizia P. Cassarà, Lorenzo Piovan, Cesare Chiosi

Improving upon the standard evolutionary population synthesis (EPS) technique, we present spectrophotometric models of galaxies whose morphology goes from spherical structures to d…

astro-ph.SR2014★ 26 cited

Exploring an Alternative Channel of Evolution Towards SNa Ia Explosion

E. Chiosi, C. Chiosi, P. Trevisan +2

In this paper we explore the possibility that isolated CO-WDs with mass smaller than the Chandrasekhar limit may undergo nuclear runaway and SNa explosion, triggered by the energy…

astro-ph.SR2014★ 27 cited

Detailed AGB evolutionary models and near infrared colours of intermediate-age stellar populations: Tests on star clusters

M. Salaris, A. Weiss, L. Cassara' +2

We investigate the influence of Asymptotic Giant Branch stars on integrated colours of star clusters of ages between ~100 Myr and a few gigayears, and composition typical for the M…

astro-ph.SR2013★ 17 cited

The Role of Dust in Models of Population Synthesis

L. P. Cassarà, L. Piovan, A. Weiss +2

We have employed state-of-the-art evolutionary models of low and intermediate-mass AGB stars, and included the effect of circumstellar dust shells on the spectral energy distributi…

astro-ph.CO2012★ 7 cited

The Origin of the Mass-Radius Relation of Early-Type Galaxies

Cesare Chiosi, Emiliano Merlin, Lorenzo Piovan

Early-type galaxies obey a narrow relation traced by their stellar content between the mass and size (Mass- Radius relation). The wealth of recently acquired observational data ess…