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2D wind clumping in hot, massive stars from hydrodynamical line-driven instability simulations using a pseudo-planar approach

Astronomy and astrophysics (Berlin), 2018-03, Vol.611, p.A17

2018

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On the spatial distribution of electron energy loss due to gyro-cooling in hot star magnetospheres

Monthly notices of the Royal Astronomical Society, 2023-08, Vol.525 (1), p.1053-1060

2023

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Mass loss from inhomogeneous hot star winds: III. An effective-opacity formalism for line radiative transfer in accelerating, clumped two-component media, and first results on theory and diagnostics

Astronomy and astrophysics (Berlin), 2014-08, Vol.568, p.1-13

2014

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Stellar envelope inflation near the Eddington limit: Implications for the radii of Wolf-Rayet stars and luminous blue variables

Astronomy and astrophysics (Berlin), 2012-02, Vol.538, p.A40

2012

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Mass and angular momentum loss via decretion disks

Astronomy and astrophysics (Berlin), 2011-03, Vol.527, p.A84

2011

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The magnetic early B-type stars – III. A main-sequence magnetic, rotational, and magnetospheric biography

Monthly notices of the Royal Astronomical Society, 2019-11, Vol.490 (1), p.274-295

2019

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Revisiting the Rigidly Rotating Magnetosphere model for Ori E – I. Observations and data analysis

Monthly notices of the Royal Astronomical Society, 2012-01, Vol.419 (2), p.959-970

2012

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On the optically thick winds of Wolf-Rayet stars

Astronomy and astrophysics (Berlin), 2017-12, Vol.608, p.A34

2017

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Magnetic massive stars as progenitors of ‘heavy’ stellar-mass black holes

Monthly notices of the Royal Astronomical Society, 2017-04, Vol.466 (1), p.1052-1060

2017

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Centrifugal breakout reconnection as the electron acceleration mechanism powering the radio magnetospheres of early-type stars

Monthly notices of the Royal Astronomical Society, 2022-04, Vol.513 (1), p.1449-1458

2022

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A rigidly rotating magnetosphere model for circumstellar emission from magnetic OB stars

Monthly notices of the Royal Astronomical Society, 2005-02, Vol.357 (1), p.251-264

2005

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The effects of surface fossil magnetic fields on massive star evolution – II. Implementation of magnetic braking in mesa and implications for the evolution of surface rotation in OB stars

Monthly notices of the Royal Astronomical Society, 2020-03, Vol.493 (1), p.518-535

2020

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The magnetic early B-type stars – IV. Breakout or leakage? H α emission as a diagnostic of plasma transport in centrifugal magnetospheres

Monthly notices of the Royal Astronomical Society, 2020-12, Vol.499 (4), p.5379-5395

2020

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Electron scattering emission in the light curves of stars with centrifugal magnetospheres

Monthly notices of the Royal Astronomical Society, 2022-03, Vol.511 (4), p.4815-4825

2022

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Mass loss from inhomogeneous hot star winds II. Constraints from a combined optical/UV study

Astronomy and astrophysics (Berlin), 2011-04, Vol.528, p.A64

2011

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MOBSTER – VII. Using light curves to infer magnetic and rotational properties of stars with centrifugal magnetospheres

Monthly notices of the Royal Astronomical Society, 2023-06, Vol.523 (4), p.6371-6385

2023

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MOBSTER – VI. The crucial influence of rotation on the radio magnetospheres of hot stars

Monthly notices of the Royal Astronomical Society, 2022-04, Vol.513 (1), p.1429-1448

2022

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Dynamically inflated wind models of classical Wolf-Rayet stars

Astronomy and astrophysics (Berlin), 2021-03, Vol.647, p.A151

2021

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Magnetic OB[A] Stars with TESS: probing their Evolutionary and Rotational properties (MOBSTER) – I. First-light observations of known magnetic B and A stars

Monthly notices of the Royal Astronomical Society, 2019-07, Vol.487 (1), p.304-317

2019

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2D simulations of the line-driven instability in hot-star winds : II. Approximations for the 2D radiation force

Astronomy and astrophysics (Berlin), 2005-07, Vol.437 (2), p.657-666

2005

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Revisiting the rigidly rotating magnetosphere model for σ Ori E – II. Magnetic Doppler imaging, arbitrary field RRM, and light variability

Monthly notices of the Royal Astronomical Society, 2015-08, Vol.451 (2), p.2015-2029

2015

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Accretion vs. colliding wind models for the gamma-ray binary LS I +61 303: an assessment

Astronomy and astrophysics (Berlin), 2007-10, Vol.474 (1), p.15-22

2007

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Detection of an extremely strong magnetic field in the double-degenerate binary merger product HD 144941

Monthly notices of the Royal Astronomical Society, 2021-10, Vol.507 (1), p.1283-1295

2021

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Line-drag damping of Alfvén waves in radiatively driven winds of magnetic massive stars

Monthly notices of the Royal Astronomical Society, 2020-12, Vol.499 (3), p.4282-4292

2020

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Populations of rotating stars: II. Rapid rotators and their link to Be-type stars

Astronomy and astrophysics (Berlin), 2013-05, Vol.553, p.1-14

2013

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2D wind clumping in hot, massive stars from hydrodynamical line-driven instability simulations using a pseudo-planar approach

On the spatial distribution of electron energy loss due to gyro-cooling in hot star magnetospheres

Mass loss from inhomogeneous hot star winds: III. An effective-opacity formalism for line radiative transfer in accelerating, clumped two-component media, and first results on theory and diagnostics

Stellar envelope inflation near the Eddington limit: Implications for the radii of Wolf-Rayet stars and luminous blue variables

Mass and angular momentum loss via decretion disks

The magnetic early B-type stars – III. A main-sequence magnetic, rotational, and magnetospheric biography

Revisiting the Rigidly Rotating Magnetosphere model for Ori E – I. Observations and data analysis

On the optically thick winds of Wolf-Rayet stars

Magnetic massive stars as progenitors of ‘heavy’ stellar-mass black holes

Centrifugal breakout reconnection as the electron acceleration mechanism powering the radio magnetospheres of early-type stars

A rigidly rotating magnetosphere model for circumstellar emission from magnetic OB stars

The effects of surface fossil magnetic fields on massive star evolution – II. Implementation of magnetic braking in mesa and implications for the evolution of surface rotation in OB stars

The magnetic early B-type stars – IV. Breakout or leakage? H α emission as a diagnostic of plasma transport in centrifugal magnetospheres

Electron scattering emission in the light curves of stars with centrifugal magnetospheres

Mass loss from inhomogeneous hot star winds II. Constraints from a combined optical/UV study

MOBSTER – VII. Using light curves to infer magnetic and rotational properties of stars with centrifugal magnetospheres

MOBSTER – VI. The crucial influence of rotation on the radio magnetospheres of hot stars

Dynamically inflated wind models of classical Wolf-Rayet stars

Magnetic OB[A] Stars with TESS: probing their Evolutionary and Rotational properties (MOBSTER) – I. First-light observations of known magnetic B and A stars

2D simulations of the line-driven instability in hot-star winds : II. Approximations for the 2D radiation force

Revisiting the rigidly rotating magnetosphere model for σ Ori E – II. Magnetic Doppler imaging, arbitrary field RRM, and light variability

Accretion vs. colliding wind models for the gamma-ray binary LS I +61 303: an assessment

Detection of an extremely strong magnetic field in the double-degenerate binary merger product HD 144941

Line-drag damping of Alfvén waves in radiatively driven winds of magnetic massive stars

Populations of rotating stars: II. Rapid rotators and their link to Be-type stars

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