54 citations · 128 across the 6 of their papers we have counts for
6 papers
Fast and accurate parameter estimation of high-redshift sources with the Einstein Telescope
Filippo Santoliquido, Jacopo Tissino, Ulyana Dupletsa +9
The Einstein Telescope (ET), along with other third-generation gravitational wave (GW) detectors, will be a key instrument for detecting GWs in the coming decades. However, analyzi…
Dynamical formation of the GW190814 merger
Manuel Arca Sedda
We investigate the possible dynamical origin of GW190814, a gravitational wave (GW) source discovered by the LIGO-Virgo-Kagra collaboration (LVC) associated with a merger between a…
On the origin of a rotating metal-poor stellar population in the Milky Way Nuclear Cluster
Manuel Arca Sedda, Alessia Gualandris, Tuan Do +3
We explore the origin of a population of stars recently detected in the inner parsec of the Milky Way Nuclear Cluster (NC), which exhibit sub-solar metallicity and a higher rotatio…
Dissecting the properties of neutron star - black hole mergers originating in dense star clusters
Manuel Arca Sedda
The detection of gravitational waves emitted during a neutron star - black hole merger and the associated electromagnetic counterpart will provide a wealth of information about ste…
The collision between the Milky Way and Andromeda and the fate of their Supermassive Black Holes
Riccardo Schiavi, Roberto Capuzzo Dolcetta, Manuel Arca Sedda +1
Our Galaxy and the nearby Andromeda Galaxy (M31) form a bound system, even though the relative velocity vector of M31 is currently not well constrained. Their orbital motion is hig…
Stellar-Mass Black Holes in Globular Clusters: Dynamical Consequences and Observational Signatures
Abbas Askar, Mirek Giersz, Manuel Arca Sedda +3
Sizeable number of stellar-mass black holes (BHs) in globular clusters (GCs) can strongly influence the dynamical evolution and observational properties of their host cluster. Usin…