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20182023
most citedMerging black hole binaries with the SEVN code

273 citations · 1.5k across the 26 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2023★ 40 cited

Nebular emission from young stellar populations including binary stars

M. Lecroq, S. Charlot, A. Bressan +8

We investigate the nebular emission produced by young stellar populations using the new GALSEVN model based on the combination of the SEVN population-synthesis code including binar…

astro-ph.SR2023

Stellar Black Holes and Compact Stellar Remnants

Guglielmo Costa, Martyna Chruślińska, Jakub Klencki +4

The recent observations of gravitational waves (GWs) by the LIGO-Virgo-KAGRA collaboration (LVK) have provided a new opportunity for studying our Universe. By detecting several mer…

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.GA2023

Dissecting the Gaia HR diagram II. The vertical structure of the star formation history across the Solar Cylinder

Alessandro Mazzi, Léo Girardi, Michele Trabucchi +11

Starting from the Gaia DR3 HR diagram, we derive the star formation history (SFH) as a function of distance from the Galactic Plane within a cylinder centred on the Sun with a 200~…

astro-ph.GA2023★ 45 cited

Binary black hole mergers from Population III stars: uncertainties from star formation and binary star properties

Filippo Santoliquido, Michela Mapelli, Giuliano Iorio +5

Population III (Pop. III) binary stars likely produced the first stellar-born binary black hole (BBH) mergers in the Universe. Here, we quantify the main sources of uncertainty for…

astro-ph.GA2023★ 29 cited

Massive binary black holes from Population II and III stars

Guglielmo Costa, Michela Mapelli, Giuliano Iorio +4

Population III stars, born from the primordial gas in the Universe, lose a negligible fraction of their mass via stellar winds and possibly follow a top-heavy mass function. Hence,…