activity
20132017
most citedVery massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

344 citations · 888 across the 8 of their papers we have counts for

collaborators

11 papers

astro-ph.GA201712 cited

The Evolution of Kicked Stellar-Mass Black Holes in Star Cluster Environments

Jeremy J. Webb, Nathan W. C. Leigh, Abhishek Singh +3

We consider how dynamical friction acts on black holes that receive a velocity kick while located at the center of a gravitational potential, analogous to a star cluster, due to ei…

astro-ph.SR2017306 cited

Merging black hole binaries: the effects of progenitor's metallicity, mass-loss rate and Eddington factor

Nicola Giacobbo, Michela Mapelli, Mario Spera

The first four gravitational wave events detected by LIGO were all interpreted as merging black hole binaries (BHBs), opening a new perspective on the study of such systems. Here w…

astro-ph.GA201724 cited

Star cluster disruption by a massive black hole binary

Elisa Bortolas, Michela Mapelli, Mario Spera

Massive black hole binaries (BHBs) are expected to form as the result of galaxy mergers; they shrink via dynamical friction and stellar scatterings, until gravitational waves (GWs)…

astro-ph.GA2017194 cited

The cosmic merger rate of stellar black hole binaries from the Illustris simulation

Michela Mapelli, Nicola Giacobbo, Emanuele Ripamonti +1

The cosmic merger rate density of black hole binaries (BHBs) can give us an essential clue to constraining the formation channels of BHBs, in light of current and forthcoming gravi…

astro-ph.SR2017344 cited

Very massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

Mario Spera, Michela Mapelli

Understanding the link between massive ( M) stellar black holes (BHs) and their progenitor stars is a crucial step to interpret observations of gravitationa…

astro-ph.GA2016

Dynamics of supernova remnants in the Galactic Centre

Elisa Bortolas, Michela Mapelli, Mario Spera

The Galactic centre (GC) is a unique place to study the extreme dynamical processes occurring near a super-massive black hole (SMBH). Here we simulate a large set of binaries orbit…