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20132023
most citedMultiple populations in globular clusters: the distinct kinematic imprints of different formation scenarios

82 citations · 495 across the 17 of their papers we have counts for

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10 papers · 1 filter

astro-ph.GA2023★ 3 cited

Multimass modelling of Milky Way globular clusters -- II. present-day black hole populations

Nolan Dickson, Peter J. Smith, Vincent Hénault-Brunet +2

Populations of stellar-mass black holes (BHs) in globular clusters (GCs) influence their dynamical evolution and have important implications on one of the main formation channels f…

astro-ph.GA2021★ 58 cited

A black hole detected in the young massive LMC cluster NGC 1850

S. Saracino, S. Kamann, M. G. Guarcello +8

We report the detection of a black hole (NGC 1850 BH1) in the 100 Myr-old massive cluster NGC~1850 in the Large Magellanic Cloud. It is in a binary system with a main-sequenc…

astro-ph.GA2019★ 42 cited

On the black hole content and initial mass function of 47 Tuc

Vincent Hénault-Brunet, Mark Gieles, Jay Strader +3

The globular cluster (GC) 47 Tuc has recently been proposed to host an intermediate-mass black hole (IMBH) or a population of stellar-mass black holes (BHs). To shed light on its d…

astro-ph.GA2018★ 31 cited

Mass modelling globular clusters in the Gaia era: a method comparison using mock data from an -body simulation of M4

Vincent Hénault-Brunet, Mark Gieles, Antonio Sollima +5

As we enter a golden age for studies of internal kinematics and dynamics of Galactic globular clusters (GCs), it is timely to assess the performance of modelling techniques in reco…

astro-ph.GA2018★ 29 cited

Linking the rotation of a cluster to the spins of its stars: The kinematics of NGC6791 and NGC6819 in 3D

Sebastian Kamann, Nate Bastian, Mark Gieles +2

The physics governing the formation of star clusters is still not entirely understood. One open question concerns the amount of angular momentum that newly formed clusters possess…

astro-ph.GA2017★ 58 cited

Radial anisotropy in omega Cen limiting the room for an intermediate-mass black hole

Alice Zocchi, Mark Gieles, Vincent Hénault-Brunet

Finding an intermediate-mass black hole (IMBH) in a globular cluster (or proving its absence) would provide valuable insights into our understanding of galaxy formation and evoluti…

astro-ph.GA2017★ 17 cited

Testing lowered isothermal models with direct N-body simulations of globular clusters - II: Multimass models

Miklos Peuten, Alice Zocchi, Mark Gieles +1

Lowered isothermal models, such as the multimass Michie-King models, have been successful in describing observational data of globular clusters. In this study we assess whether suc…

astro-ph.GA2016★ 45 cited

Testing lowered isothermal models with direct N-body simulations of globular clusters

Alice Zocchi, Mark Gieles, Vincent Hénault-Brunet +1

Several self-consistent models have been proposed, aiming at describing the phase space distribution of stars in globular clusters. This study explores the ability of the recently…

astro-ph.GA2016★ 20 cited

No evidence for younger stellar generations within the intermediate age massive clusters NGC 1783, NGC 1696 and NGC 411

I. Cabrera-Ziri, F. Niederhofer, N. Bastian +11

Recently, Li et al. (2016) claimed to have found evidence for multiple generations of stars in the intermediate age clusters NGC 1783, NGC 1696 and NGC 411 in the Large and Small M…

astro-ph.GA2015★ 82 cited

Multiple populations in globular clusters: the distinct kinematic imprints of different formation scenarios

Vincent Hénault-Brunet, Mark Gieles, Oscar Agertz +1

Several scenarios have been proposed to explain the presence of multiple stellar populations in globular clusters. Many of them invoke multiple generations of stars to explain the…