activity
20162020
collaborators

5 papers

astro-ph.HE2020

Binary black holes in young star clusters: the impact of metallicity

Ugo N. Di Carlo, Michela Mapelli, Nicola Giacobbo +9

Young star clusters are the most common birth-place of massive stars and are dynamically active environments. Here, we study the formation of black holes (BHs) and binary black hol…

astro-ph.HE2020

Dynamics of black hole - neutron star binaries in young star clusters

Sara Rastello, Michela Mapelli, Ugo N. Di Carlo +5

Young star clusters are likely the most common birthplace of massive stars across cosmic time and influence the formation of compact binaries in several ways. Here, we simulate the…

astro-ph.GA2020

Evolution of fractality and rotation in embedded star clusters

Alessandro Ballone, Michela Mapelli, Ugo N. Di Carlo +3

More and more observations indicate that young star clusters could retain imprints of their formation process. In particular, the degree of substructuring and rotation are possibly…

astro-ph.GA2019

A common origin for the circumnuclear disc and the nearby molecular clouds in the Galactic Centre

Alessandro Ballone, Michela Mapelli, Alessandro Alberto Trani

The origin of the molecular clouds orbiting SgrA* is one of the most debated questions about our Galactic Centre. Here, we present the hydrodynamic simulation of a molecular cloud…

astro-ph.GA2016

The G2+G2t complex as a fast and massive outflow?

A. Ballone, M. Schartmann, A. Burkert +8

Observations of the gas component of the cloud G2 in the Galactic Center have revealed its connection to a tail (G2t) lying on the same orbit. More recent studies indicate a connec…