66 citations · 106 across the 16 of their papers we have counts for
21 papers
Shaping binary black hole merger efficiency with gravitational wave observations
Michele Bosi, Lumen Boco, Stefano Torniamenti +5
Gravitational wave (GW) astronomy offers unprecedented insights into binary black hole (BBH) coalescence. However, many of the key quantities involved remain inaccessible to direct…
N/O-enhanced chemical enrichment by massive stars: the interplay of optically-thick winds and rotation
Boyuan Liu, Michela Mapelli, Lumen Boco +1
Recent JWST observations have revealed a sample of high- galaxies with highly enhanced N/O abundance ratios, . Strong optically-thick winds of rotatin…
Breaking binary formation mechanism degeneracies with gravitational wave clustering
Nicola Bellomo, Michele Bosi, Sarah Libanore +4
Thanks to the almost 400 gravitational wave events detected, we are currently able to grasp the fundamental features of black hole mass, spin, and distance distributions. However,…
Exploring the connection between Fast Radio Bursts and binary neutron star mergers
Barbara Patricelli, Maria Grazia Bernardini, Cecilia Sgalletta +1
Fast Radio Bursts (FRBs) are highly energetic radio sources whose duration is of the order of milliseconds. The physical origin of these sources is still unknown. Many models sugge…
Linking high-mass X-ray binaries to binary compact object mergers in Milky Way-like galaxies
Felipe Vivanco Cádiz, M. Celeste Artale, Nicola Masetti +5
High-mass X-ray binaries (HMXBs) constitute a potential intermediate phase connecting massive stellar binaries to the formation of coalescing binary compact objects (BCOs). Yet, th…
A binary black hole merger rate comparison within the same metallicity - star formation rate framework
Lumen Boco, Michele Bosi, Cecilia Sgalletta +2
Recent studies have suggested that binary population synthesis models, when coupled with observationally based, metallicity-dependent star formation rate density, overpredict the o…