activity
20242026
collaborators

7 papers

astro-ph.HE2026

The impact of stellar binaries and star cluster dynamics on pair-instability supernovae

Francesco Gabrielli, Cristiano Ugolini, Lavinia Paiella +12

Pair-instability supernovae (PISNe) are among the most luminous transients in the Universe. However, they have never been confidently observed. Solving this puzzle would have key i…

astro-ph.SR2026

The impact of envelope binding energies on the merger rate density of binary compact objects

Cecilia Sgalletta, Guglielmo Costa, Giuliano Iorio +8

The common envelope (CE) phase plays a key role in the formation of binary compact object systems. Its final outcome strongly depends on the envelope binding energy, but this quant…

astro-ph.GA2026

Impact of initial mass function on the chemical evolution of high-redshift galaxies

Boyuan Liu, Michela Mapelli, Volker Bromm +10

Recent observations by the James Webb Space Telescope (JWST) have found evidence for an invariant relation between stellar mass, metallicity, and star formation rate up to $z\sim 8…

astro-ph.SR2025

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…

astro-ph.SR2025

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

A new prescription for the spectral properties of population III stellar populations

Marie Lecroq, Stéphane Charlot, Alessandro Bressan +7

We investigated various emission properties of extremely low metallicity stellar populations in the Epoch of Reionization (EoR), using the new GALSEVN model, which has shown promis…