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A stellar-mass black hole population in the globular cluster NGC 6101?

Monthly notices of the Royal Astronomical Society, 2016-11, Vol.462 (3), p.2333-2342

2016

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

Monthly notices of the Royal Astronomical Society, 2017-09, Vol.470 (3), p.2736-2761

2017

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No evidence for younger stellar generations within the intermediate-age massive clusters NGC 1783, NGC 1806 and NGC 411

Monthly notices of the Royal Astronomical Society, 2016-07, Vol.459 (4), p.4218-4223

2016

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Binary-corrected velocity dispersions from single- and multi-epoch radial velocities: massive stars in R136 as a test case

Astronomy and astrophysics (Berlin), 2014-02, Vol.562, p.np-np

2014

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Evidence for a bottom-light initial mass function in massive star clusters

Monthly notices of the Royal Astronomical Society, 2023-05, Vol.521 (3), p.3991-4008

2023

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

Monthly notices of the Royal Astronomical Society, 2022-02, Vol.511 (2), p.2914-2924

2022

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Discovery of a Be/X‐ray pulsar binary and associated supernova remnant in the Wing of the Small Magellanic Cloud

Monthly notices of the Royal Astronomical Society. Letters, 2012-02, Vol.420 (1), p.L13-L17

2012

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Multimass modelling of Milky Way globular clusters – I. Implications on their stellar initial mass function above 1 M

Monthly notices of the Royal Astronomical Society, 2023-05, Vol.522 (4), p.5320-5339

2023

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Multimass modelling of milky way globular clusters – II. Present-day black hole populations

Monthly notices of the Royal Astronomical Society, 2024-02, Vol.529 (1), p.331-347

2024

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A Massive Runaway Star from 30 Doradus

Astrophysical journal. Letters, 2010-06, Vol.715 (2), p.L74-L79

2010

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The VLT-FLAMES Tarantula Survey: The Fastest Rotating O-type Star and Shortest Period LMC Pulsar—Remnants of a Supernova Disrupted Binary?

Astrophysical journal. Letters, 2011-12, Vol.743 (1), p.L22-jQuery1323914587255='48'

2011

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Mass modelling globular clusters in the Gaia era: a method comparison using mock data from an N -body simulation of M 4

Monthly notices of the Royal Astronomical Society, 2019-02, Vol.483 (1), p.1400-1425

2019

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

Monthly notices of the Royal Astronomical Society, 2015-06, Vol.450 (2), p.1164-1198

2015

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Differences in the rotational properties of multiple stellar populations in M13: a faster rotation for the ‘extreme’ chemical subpopulation

Monthly notices of the Royal Astronomical Society, 2017-03, Vol.465 (3), p.3515-3515

2017

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An excess of massive stars in the local 30 Doradus starburst

Science (American Association for the Advancement of Science), 2018-01, Vol.359 (6371), p.69-71

2018

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

Monthly notices of the Royal Astronomical Society, 2020-01, Vol.491 (1), p.113-128

2020

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Globular cluster number density profiles using Gaia DR2

Monthly notices of the Royal Astronomical Society, 2019-06, Vol.485 (4), p.4906-4935

2019

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Biases in the determination of dynamical parameters of star clusters: today and in the Gaia era

Monthly notices of the Royal Astronomical Society, 2015-08, Vol.451 (2), p.2185-2197

2015

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The VLT-FLAMES Tarantula Survey: VIII. Multiplicity properties of the O-type star population

Astronomy and astrophysics (Berlin), 2013-02, Vol.550, p.1-22

2013

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Space astrometry of the very massive ∼150 M⊙ candidate runaway star VFTS682

Monthly notices of the Royal Astronomical Society. Letters, 2019-01, Vol.482 (1), p.L102-L106

2019

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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

Monthly notices of the Royal Astronomical Society, 2019-02, Vol.483 (2), p.2197-2206

2019

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Studying the kinematics of the giant star-forming region 30 Doradus: I. The data

Astronomy and astrophysics (Berlin), 2013-07, Vol.555, p.np-np

2013

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The VLT-FLAMES Tarantula Survey: XXI. Stellar spin rates of O-type spectroscopic binaries

Astronomy and astrophysics (Berlin), 2015-08, Vol.580, p.A92

2015

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Long-term evolution of the neutron-star spin period of SXP 1062

Astronomy and astrophysics (Berlin), 2013-08, Vol.556, p.1-8

2013

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A closer look at the binary content of NGC 1850

Monthly notices of the Royal Astronomical Society, 2023-11, Vol.526 (1), p.299-322

2023

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A stellar-mass black hole population in the globular cluster NGC 6101?

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

No evidence for younger stellar generations within the intermediate-age massive clusters NGC 1783, NGC 1806 and NGC 411

Binary-corrected velocity dispersions from single- and multi-epoch radial velocities: massive stars in R136 as a test case

Evidence for a bottom-light initial mass function in massive star clusters

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

Discovery of a Be/X‐ray pulsar binary and associated supernova remnant in the Wing of the Small Magellanic Cloud

Multimass modelling of Milky Way globular clusters – I. Implications on their stellar initial mass function above 1 M

Multimass modelling of milky way globular clusters – II. Present-day black hole populations

A Massive Runaway Star from 30 Doradus

The VLT-FLAMES Tarantula Survey: The Fastest Rotating O-type Star and Shortest Period LMC Pulsar—Remnants of a Supernova Disrupted Binary?

Mass modelling globular clusters in the Gaia era: a method comparison using mock data from an N -body simulation of M 4

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

Differences in the rotational properties of multiple stellar populations in M13: a faster rotation for the ‘extreme’ chemical subpopulation

An excess of massive stars in the local 30 Doradus starburst

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

Globular cluster number density profiles using Gaia DR2

Biases in the determination of dynamical parameters of star clusters: today and in the Gaia era

The VLT-FLAMES Tarantula Survey: VIII. Multiplicity properties of the O-type star population

Space astrometry of the very massive ∼150 M⊙ candidate runaway star VFTS682

Linking the rotation of a cluster to the spins of its stars: the kinematics of NGC 6791 and NGC 6819 in 3D

Studying the kinematics of the giant star-forming region 30 Doradus: I. The data

The VLT-FLAMES Tarantula Survey: XXI. Stellar spin rates of O-type spectroscopic binaries

Long-term evolution of the neutron-star spin period of SXP 1062

A closer look at the binary content of NGC 1850

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