Vincent Hénault-Brunet
educated at: University of Edinburgh
occupation: researcher
Articles 52
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An X-ray-quiet black hole born with a negligible kick in a massive binary within the Large Magellanic Cloud
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MUSE narrow field mode observations of the central kinematics of M15
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Globular cluster number density profiles using Gaia DR2
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Shape coexistence in 94Zr studied via Coulomb excitation
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An excess of massive stars in the local 30 Doradus starburst.
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The Unexpected Kinematics of Multiple Populations in NGC 6362: Do Binaries Play a Role?
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Linking the rotation of a cluster to the spins of its stars: The kinematics of NGC 6791 and NGC 6819 in 3D
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Concurrent formation of supermassive stars and globular clusters: implications for early self-enrichment
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The effect of stellar-mass black holes on the central kinematics of ω Cen: a cautionary tale for IMBH interpretations
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Response to Comment on “An excess of massive stars in the local 30 Doradus starburst”
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Mass modelling globular clusters in the Gaiaera: a method comparison using mock data from an N-body simulation of M 4
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Space astrometry of the very massive ∼150 M⊙ candidate runaway star VFTS682
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The Tarantula Massive Binary Monitoring
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Mass models of NGC 6624 without an intermediate-mass black hole
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Testing lowered isothermal models with direct N-body simulations of globular clusters – II. Multimass models
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A stellar-mass black hole population in the globular cluster NGC 6101?
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No evidence for younger stellar generations within the intermediate-age massive clusters NGC 1783, NGC 1806 and NGC 411
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Testing lowered isothermal models with directN-body simulations of globular clusters
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Differences in the rotational properties of multiple stellar populations in M13: a faster rotation for the ‘extreme’ chemical subpopulation
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The spectral variability of a sample of WC 9 stars on time-scales of days to weeks
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Chemistry and kinematics of red supergiant stars in the young massive cluster NGC 2100
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Biases in the determination of dynamical parameters of star clusters: today and in the Gaia era
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The VLT-FLAMES Tarantula Survey. XXI. Stellar spin rates of O-type spectroscopic binaries
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The VLT-FLAMES Tarantula Survey. XIX. B-type supergiants: Atmospheric parameters and nitrogen abundances to investigate the role of binarity and the width of the main sequence
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The VLT-FLAMES Tarantula Survey. XVIII. Classifications and radial velocities of the B-type stars
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Multiple populations in globular clusters: the distinct kinematic imprints of different formation scenarios
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Multiple populations in globular clusters: constraints from kinematics and dynamics
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The VLT-FLAMES Tarantula Survey. XVII. Physical and wind properties of massive stars at the top of the main sequence
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On the uniqueness of kinematical signatures of intermediate-mass black holes in globular clusters
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Binary-corrected velocity dispersions from single- and multi-epoch radial velocities: massive stars in R136 as a test case
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The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population
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Discovery of X-ray emission from young suns in the Small Magellanic Cloud
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