activity
20082024
most citedMerging black holes in young star clusters

271 citations · 843 across the 25 of their papers we have counts for

collaborators
Showing 2019 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2019★ 54 cited

Mass and star formation rate of the host galaxies of compact binary mergers across cosmic time

M. Celeste Artale, Michela Mapelli, Yann Bouffanais +3

We investigate the properties of the host galaxies of compact binary mergers across cosmic time, by means of population-synthesis simulations combined with galaxy catalogues from t…

astro-ph.GA2019

Radial Dependence of the Proto-Globular Cluster Contribution to the Milky Way Formation

Chul Chung, Mario Pasquato, Sang-Yoon Lee +4

Recent interpretation of the colormagnitude diagrams of the Milky Way (MW) bulge has suggested that the observed double red-clump feature can be a natural consequence of He-enha…

astro-ph.GA2019

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…

astro-ph.GA2019

Further properties of the dynamical clock A+ indicator in a toy model of pure dynamical friction

Mario Pasquato

The Alessandrini A indicator is a quantitative measure of star cluster dynamical evolution based on the mass-segregation of blue straggler stars. A is defined as the integral…

astro-ph.GA2019

Analytical solutions for the dynamical clock A+ indicator in a toy model of pure dynamical friction

Mario Pasquato

Blue straggler stars are more massive than the average star in globular clusters, as they originate from the merger of two stars. Consequently, they experience dynamical friction,…

astro-ph.GA2019

Clustering clusters: unsupervised machine learning on globular cluster structural parameters

Mario Pasquato, Chul Chung

Globular Clusters (GCs) have historically been subdivided in either two (disk/halo) or three (disk/inner-halo/outer-halo) groups based on their orbital, chemical and internal physi…