activity
20092026
most citedYields of AGB and SAGB models with chemistry of low- and high-metallicity Globular Clusters

284 citations · 3.1k across the 55 of their papers we have counts for

collaborators
Showing 2014Show all

5 papers · 1 filter

astro-ph.SR2014★ 75 cited

AGB stars in the LMC: evolution of dust in circumstellar envelopes

F. Dell'Agli, P. Ventura, R. Schneider +4

We calculated theoretical evolutionary sequences of asymptotic giant branch (AGB) stars, including formation and evolution of dust grains in their circumstellar envelope. By consid…

astro-ph.GA2014★ 110 cited

The dust production rate of AGB stars in the Magellanic Clouds

Raffaella Schneider, Rosa Valiante, Paolo Ventura +4

We compare theoretical dust yields for stars with mass 1 Msun < mstar < 8 Msun, and metallicities 0.001 < Z < 0.008 with observed dust production rates (DPR) by carbon- rich and ox…

astro-ph.SR2014★ 39 cited

On the alumina dust production in the winds of O-rich Asymptotic Giant Branch stars

F. Dell'Agli, D. A. García-Hernández, C. Rossi +3

The O-rich Asymptotic Giant Branch (AGB) stars experience strong mass loss with efficient dust condensation and they are major sources of dust in the interstellar medium. Alumina d…

astro-ph.SR2014★ 37 cited

Dissecting the Spitzer color-magnitude diagrams of extreme LMC AGB stars

F. Dell'Agli, P. Ventura, D. A. García Hernández +5

We trace the full evolution of low- and intermediate-mass stars () during the Asymptotic Giant Branch (AGB) phase in the {\it Spitzer} two-color…

astro-ph.SR2014★ 106 cited

Dust from AGBs: relevant factors and modelling uncertainties

P. Ventura, F. Dell'Agli, R. Schneider +5

The dust formation process in the winds of Asymptotic Giant Branch stars is discussed, based on full evolutionary models of stars with mass in the range MM$\leq 8…