collaborators

5 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.GA2026

Mirror images of lensed star clusters with mismatched spectral energy distributions: A possible signature of top-heavy stellar initial mass functions and extreme stars in high-redshift star clusters

Erik Zackrisson, Jose M. Diego, Jose M. Palencia +4

Strongly lensed star clusters have recently been detected up to redshift in galaxy cluster fields using the James Webb Space Telescope (JWST). When pairs of mirror im…

astro-ph.HE2024

Constraining the Initial-Mass Function via Stellar Transients

Francesco Gabrielli, Lumen Boco, Giancarlo Ghirlanda +4

The stellar initial-mass function (IMF) represents a fundamental quantity in astrophysics and cosmology, describing the mass distribution of stars from low to very-high masses. It…

astro-ph.HE2024

The cosmic rate of Pair-Instability Supernovae

Francesco Gabrielli, Andrea Lapi, Lumen Boco +8

Pair-instability supernovae (PISNe) have crucial implications for many astrophysical topics, including the search for very massive stars, the black hole mass spectrum, and galaxy c…

astro-ph.HE2024

Multi-messenger prospects for black hole - neutron star mergers in the O4 and O5 runs

Alberto Colombo, Raphaël Duqué, Om Sharan Salafia +13

The existence of merging black hole-neutron star (BHNS) binaries has been ascertained through the observation of their gravitational wave (GW) signals. However, to date, no definit…