activity
20172023
most citedAGB and SAGB stars: modelling dust production at solar metallicity

51 citations · 172 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2023

Dust from evolved stars: a pilot analysis of the AGB to PN transition

F. Dell'Agli, S. Tosi, D. Kamath +5

We present a novel approach to address dust production by low- and intermediate-mass stars. We study the asymptotic giant branch (AGB) phase, during which the formation of dust tak…

astro-ph.SR2023★ 2 cited

An insight into Capella (alpha Aurigae): from the extent of core overshoot to its evolutionary history

E. Marini, C. Ventura, M. Tailo +3

The binary star alpha Aurigae (otherwise known as Capella) is extremely important to understand the core hydrogen and helium burning phases of the stars, as the primary star is lik…

astro-ph.SR2021

Gas and dust from extremely metal-poor AGB stars

P. Ventura, F. Dell'Agli, D. Romano +8

We study the evolution of extremely metal-poor AGB stars, with metallicities down to [Fe/H]=-5, to understand the main evolutionary properties, the efficiency of the processes able…

astro-ph.SR2020★ 30 cited

Understanding the evolution and dust formation of carbon stars in the LMC with a look at the JWST

E. Marini, F. Dell'Agli, M. A. T. Groenewegen +6

Carbon stars have been and are extensively studied, given their complex internal structure and their peculiar chemical composition, which make them living laboratories to test stel…

astro-ph.SR2020★ 13 cited

Are extreme AGB stars post-common envelope binaries?

F. Dell'Agli, E. Marini, F. D'Antona +6

Modelling dust formation in single stars evolving through the carbon-star stage of the asymptotic giant branch (AGB) reproduces well the mid-infrared colours and magnitudes of most…

astro-ph.SR2020★ 12 cited

Characterization of M-stars in the LMC in the JWST era

E. Marini, F. Dell'Agli, M. Di Criscienzo +8

We study the M-type asymptotic giant branch (AGB) population of the Large Magellanic Cloud (LMC) by characterizing the individual sources in terms of the main properties of the pro…