activity
20242026
most citedEvolutionary tracks, ejecta, and ionizing photons from intermediate-mass to very massive stars with PARSEC

33 citations · 50 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026★ 1 cited

Not all nitrogen-rich field stars originate from globular clusters

Ellen I. Leitinger, Andrea Miglio, Josefina Montalbán +7

Globular clusters (GCs) are important tracers of the early Galactic assembly process, with part of their stars showing distinct chemical abundance patterns. When such stars are fou…

astro-ph.SR2025★ 2 cited

Inferring the efficiency of convective-envelope overshooting in Red Giant Branch stars

Lorenzo Briganti, Marco Tailo, Edoardo Ceccarelli +6

The understanding of mixing processes in stars is crucial for improving our knowledge of the chemical abundances in stellar photospheres and of their variation with evolutionary ph…

astro-ph.SR2025★ 7 cited

DUETS: Setting expectations for asteroseismic binaries and binary products with synthetic populations

A. Mazzi, J. S. Thomsen, A. Miglio +5

Asteroseismology gives us the opportunity to better characterize binaries and their products, and shed light on their role in Galactic populations. We estimate occurrence rates, ma…

astro-ph.SR2025★ 33 cited

Evolutionary tracks, ejecta, and ionizing photons from intermediate-mass to very massive stars with PARSEC

G. Costa, K. G. Shepherd, A. Bressan +12

Recent advancements in stellar evolution modeling offer unprecedented accuracy in predicting the evolution and deaths of stars. We present new stellar evolutionary models computed…

astro-ph.SR2024★ 7 cited

Anomalously low-mass core-He-burning star in NGC 6819 as a post-common-envelope phase product

Massimiliano Matteuzzi, David Hendriks, Robert G. Izzard +5

Precise masses of red-giant stars enable a robust inference of their ages, but there are cases where these age estimates are highly precise yet very inaccurate. Examples are core-h…