[HTML][HTML] Gas and dust from extremely metal-poor AGB stars
P Ventura, F Dell'Agli, D Romano, S Tosi… - Astronomy & …, 2021 - aanda.org
Context. The study of stars that evolve through the asymptotic giant branch (AGB) proves
crucial in several astrophysical contexts because these objects provide important feedback …
crucial in several astrophysical contexts because these objects provide important feedback …
Gas and dust from extremely metal-poor AGB stars
P Ventura, F Dell'agli, D Romano… - Astronomy and …, 2021 - lanlexperts.elsevierpure.com
Context. The study of stars that evolve through the asymptotic giant branch (AGB) proves
crucial in several astrophysical contexts because these objects provide important feedback …
crucial in several astrophysical contexts because these objects provide important feedback …
[PDF][PDF] Gas and dust from extremely metal-poor AGB stars
P Ventura, F Dell'Agli, D Romano, S Tosi… - ASTRONOMY & …, 2021 - real.mtak.hu
Context. The study of stars evolving through the asymptotic giant branch (AGB) proves
crucial in several astrophysical contexts, given the important feedback provided by these …
crucial in several astrophysical contexts, given the important feedback provided by these …
[PDF][PDF] Gas and dust from extremely metal-poor AGB stars
P Ventura, F Dell'Agli, D Romano, S Tosi, M Limongi… - A&A, 2021 - researchgate.net
Context. The study of stars that evolve through the asymptotic giant branch (AGB) proves
crucial in several astrophysical contexts because these objects provide important feedback …
crucial in several astrophysical contexts because these objects provide important feedback …
Gas and dust from extremely metal-poor AGB stars
P Ventura, F Dell'Agli, D Romano, S Tosi… - arXiv preprint arXiv …, 2021 - arxiv.org
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 to …
5, to understand the main evolutionary properties, the efficiency of the processes able to …
[PDF][PDF] Gas and dust from extremely metal-poor AGB stars
P Ventura, F Dell'Agli, D Romano, S Tosi, M Limongi… - 2021 - research.iac.es
Context. The study of stars evolving through the asymptotic giant branch (AGB) proves
crucial in several astrophysical contexts, given the important feedback provided by these …
crucial in several astrophysical contexts, given the important feedback provided by these …
[PDF][PDF] Gas and dust from extremely metal-poor AGB stars
P Ventura, F Dell'Agli, D Romano, S Tosi, M Limongi… - A&A, 2021 - scholar.archive.org
Context. The study of stars that evolve through the asymptotic giant branch (AGB) proves
crucial in several astrophysical contexts because these objects provide important feedback …
crucial in several astrophysical contexts because these objects provide important feedback …
Gas and dust from extremely metal-poor AGB stars
P Ventura, F Dell'Agli, D Romano… - Astronomy and …, 2021 - ui.adsabs.harvard.edu
Context. The study of stars that evolve through the asymptotic giant branch (AGB) proves
crucial in several astrophysical contexts because these objects provide important feedback …
crucial in several astrophysical contexts because these objects provide important feedback …
Gas and dust from extremely metal-poor AGB stars
P Ventura, F Dell'Agli, D Romano, S Tosi… - Astronomy and …, 2021 - diva-portal.org
Context. The study of stars that evolve through the asymptotic giant branch (AGB) proves
crucial in several astrophysical contexts because these objects provide important feedback …
crucial in several astrophysical contexts because these objects provide important feedback …
Gas and dust from extremely metal-poor AGB stars
P Ventura, F Dell'Agli, D Romano, S Tosi… - Astronomy and …, 2021 - diva-portal.org
Aims. We study the evolution of extremely metal-poor AGB stars with metallicities down to
[Fe/H]=− 5 to understand the main evolutionary properties and the efficiency of the …
[Fe/H]=− 5 to understand the main evolutionary properties and the efficiency of the …