activity
20152022
most citedMultiple populations in globular clusters: the distinct kinematic imprints of different formation scenarios

82 citations · 149 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph.SR202230 cited

The VLT-FLAMES Tarantula Survey: Observational evidence for two distinct populations of massive runaway stars in 30 Doradus

H. Sana, O. H. Ramírez-Agudelo, V. Hénault-Brunet +17

Two main scenarios have been proposed for origin of massive runaway stars -- dynamical ejection or release from a binary at the first core collapse -- but their relative contributi…

astro-ph.IM2019

Astronomy in a Low-Carbon Future

Christopher D. Matzner, Nicolas B. Cowan, René Doyon +12

The global climate crisis poses new risks to humanity, and with them, new challenges to the practices of professional astronomy. Avoiding the more catastrophic consequences of glob…

astro-ph.GA2019

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.IM201937 cited

The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition

The MSE Science Team, Carine Babusiaux, Maria Bergemann +258

(Abridged) The Maunakea Spectroscopic Explorer (MSE) is an end-to-end science platform for the design, execution and scientific exploitation of spectroscopic surveys. It will unvei…

astro-ph.GA2018

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

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…