activity
20222026
most citedPARSEC V2.0: Stellar tracks and isochrones of low and intermediate mass stars with rotation

186 citations · 290 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026

Something new under the Sun: A magnetically driven CH/CN anti-correlation

Y. Momany, L. Monaco, S. Villanova +11

Spectroscopic monitoring surveys have shown that the magnetic cycle alters the photospheric structure of the Sun, perturbing the formation of molecular lines. In parallel, the stud…

astro-ph.SR2025★ 12 cited

PARSEC V2.0: Rotating tracks and isochrones for seven addtional metallicities in the range Z=0.0001-0.03

C. T. Nguyen, G. Costa, A. Bressan +10

PARSEC v2.0 rotating stellar tracks were previously presented for six values of metallicity from subsolar to solar values, with initial rotation rates (, defined as t…

astro-ph.SR2025★ 5 cited

Enhanced Mass Loss of Very Massive Stars: Impact on the Evolution, Binary Processes, and Remnant Mass Spectrum

Kendall G. Shepherd, Guglielmo Costa, Cristiano Ugolini +7

Very massive stars (VMS) play a fundamental role in astrophysics due to their winds and supernovae (SN), and their role as massive black hole (BH) progenitors. However, their origi…

astro-ph.GA2025★ 1 cited

Strikingly high fraction of fast rotators in Magellanic Cloud star clusters

Greta Ettorre, Alessandro Mazzi, Leo Girardi +14

There has been growing evidence that the rich star clusters in the Magellanic Clouds contain significant fractions of rapidly rotating stars. In this work, we aim to constrain thes…

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

AESOPUS 2.1: Low-Temperature Opacities Extended to High Pressure

Paola Marigo, Francesco Addari, Diego Bossini +5

We address the critical need for accurate Rosseland mean gas opacities in high-pressure environments, spanning temperatures from 100 K to 32000 K. Current opacity tables from Wichi…

astro-ph.SR2024★ 10 cited

The Impact of the Third Dredge-up and Mass Loss in Shaping the Initial-Final Mass Relation of White Dwarfs

Francesco Addari, Paola Marigo, Alessandro Bressan +3

The initial-final mass relation (IFMR) plays a crucial role in understanding stellar structure and evolution by linking a star's initial mass to the mass of the resulting white dwa…

astro-ph.GA2023★ 1 cited

The detection and characterization of highly magnified stars with JWST: Prospects of finding Population III

Erik Zackrisson, Adam Hultquist, Aron Kordt +10

Gravitational lensing may render individual high-mass stars detectable out to cosmological distances, and several extremely magnified stars have in recent years been detected out t…

astro-ph.HE2023★ 10 cited

A Study of Primordial Very Massive Star Evolution. II. Stellar Rotation and Gamma-Ray Burst Progenitors

Guglielmo Volpato, Paola Marigo, Guglielmo Costa +4

We calculate new evolutionary models of rotating primordial very massive stars, with initial mass from to , for two values of the initial metallici…

astro-ph.SR2022★ 32 cited

A Study of Primordial Very Massive Star Evolution

Guglielmo Volpato, Paola Marigo, Guglielmo Costa +3

We present new evolutionary models of primordial very massive stars, with initial masses ranging from to , that extend from…

astro-ph.SR2022★ 186 cited

PARSEC V2.0: Stellar tracks and isochrones of low and intermediate mass stars with rotation

C. T. Nguyen, G. Costa, L. Girardi +6

We present a new comprehensive collection of stellar evolutionary tracks and isochrones for rotating low- and intermediate-mass stars assembled with the updated version of PARSEC V…