activity
20182021
most citedUnderstanding the evolution and dust formation of carbon stars in the LMC with a look at the JWST

30 citations · 61 across the 5 of their papers we have counts for

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Showing astro-ph.SRShow all

8 papers · 1 filter

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.SR202030 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.SR202013 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.SR202012 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…

astro-ph.SR20196 cited

Do evolved stars in the LMC show dual dust chemistry?

E. Marini, F. Dell'Agli, D. A. García-Hernández +4

We study a group of evolved M-stars in the Large Magellanic Cloud, characterized by a peculiar spectral energy distribution. While the m feature arises from silicate particl…

astro-ph.SR2018

The Gaia-LSST Synergy: resolved stellar populations in selected Local Group stellar systems

G. Clementini, I. Musella, A. Chieffi +18

This project aims at exploiting the wide-field and limiting-magnitude capabilities of the LSST to fully characterise the resolved stellar populations in/around six Local Group stel…