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20082024
most citedMerging black holes in young star clusters

271 citations · 1.5k across the 52 of their papers we have counts for

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Showing 2021Show all

6 papers · 1 filter

astro-ph.GA2021★ 32 cited

Disruption of Hierarchical Clustering in the Vela OB2 Complex and the Cluster Pair Collinder 135 and UBC7 with Gaia EDR3: Evidence of Supernova Quenching

Xiaoying Pang, Zeqiu Yu, Shih-Yun Tang +4

We identify hierarchical structures in the Vela OB2 complex and the cluster pair Collinder 135 and UBC 7 with Gaia EDR3 using the neural network machine learning algorithm StarGO.…

astro-ph.GA2021★ 82 cited

Intermediate mass black holes from stellar mergers in young star clusters

Ugo N. Di Carlo, Michela Mapelli, Mario Pasquato +8

Intermediate mass black holes (IMBHs) in the mass range bridge the gap between stellar black holes (BHs) and supermassive BHs. Here, we investigate…

astro-ph.GA2021★ 11 cited

The impact of binaries on the evolution of star clusters from turbulent molecular clouds

Stefano Torniamenti, Alessandro Ballone, Michela Mapelli +5

Most of massive stars form in binary or higher-order systems in clumpy, sub-structured clusters. In the very first phases of their life, these stars are expected to interact with t…

astro-ph.GA2021★ 16 cited

Interpreting automatic AGN classifiers with saliency maps

T. Peruzzi, M. Pasquato, S. Ciroi +3

The classification of the optical spectra of active galactic nuclei (AGN) into different types is well founded on AGN physics, but it involves some degree of human oversight and ca…

astro-ph.GA2021★ 2 cited

Introducing a new multi-particle collision method for the evolution of dense stellar systems II. Core collapse

Pierfrancesco Di Cintio, Mario Pasquato, Alicia Simon-Petit +1

In a previous paper we introduced a new method for simulating collisional gravitational -body systems with linear time scaling on , based on the Multi-Particle Collision (MPC…

astro-ph.GA2021★ 81 cited

3D Morphology of Open Clusters in the Solar Neighborhood with Gaia EDR3: its Relation to Cluster Dynamics

Xiaoying Pang, Yuqian Li, Zeqiu Yu +5

We analyze the 3D morphology and kinematics of 13 open clusters (OCs) located within 500 pc of the Sun, using Gaia EDR3 and kinematic data from literature. Members of OCs are ident…