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Isochrone fitting of the open cluster M67 in the era of Gaia and improved model physics

Monthly notices of the Royal Astronomical Society, 2024-08, Vol.532 (2), p.2860-2874

2024

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A GRID OF THREE-DIMENSIONAL STELLAR ATMOSPHERE MODELS OF SOLAR METALLICITY. I. GENERAL PROPERTIES, GRANULATION, AND ATMOSPHERIC EXPANSION

The Astrophysical journal, 2013-05, Vol.769 (1), p.1-15

2013

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The Stagger Code for Accurate and Efficient, Radiation-coupled Magnetohydrodynamic Simulations

The Astrophysical journal, 2024-07, Vol.970 (1), p.24

2024

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Does the νmax Scaling Relation Depend on Metallicity? Insights from 3D Convection Simulations

The Astrophysical journal, 2024-02, Vol.962 (2), p.118

2024

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An opaque Sun? The potential for future, higher opacities to solve the solar abundance problem

EPJ Web of Conferences, 2017, Vol.160, p.2005

2017

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Improving 1D Stellar Models with 3D Atmospheres

EPJ Web of Conferences, 2017, Vol.160, p.3009

2017

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ON THE AMPLITUDE OF CONVECTIVE VELOCITIES IN THE DEEP SOLAR INTERIOR

The Astrophysical journal, 2012-10, Vol.757 (2), p.128

2012

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Modeling the Near-Surface Shear Layer: Diffusion Schemes Studied With CSS

Journal of physics. Conference series, 2011-01, Vol.271 (1), p.012070-4

2011

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The Surface of Stellar Models - Now with more 3D simulations

EPJ Web of Conferences, 2015, Vol.101, p.6064-1-06064-2

2015

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The elemental composition of the Sun: I. The intermediate mass elements Na to Ca

Astronomy and astrophysics (Berlin), 2015-01, Vol.573, p.A25

2015

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Improvements to stellar structure models, based on a grid of 3D convection simulations – II. Calibrating the mixing-length formulation

Monthly notices of the Royal Astronomical Society, 2014-12, Vol.445 (4), p.4366-4384

2014

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The Mass Mixing Length in Convective Stellar Envelopes

The Astrophysical journal, 2011-04, Vol.731 (2), p.78-jQuery1323909216036='48'

2011

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Improvements to stellar structure models, based on a grid of 3D convection simulations – I. T(τ) relations

Monthly notices of the Royal Astronomical Society, 2014-07, Vol.442 (1), p.805-820

2014

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Three-dimensional hydrodynamical simulations of surface convection in red giant stars : Impact on spectral line formation and abundance analysis

Astronomy and astrophysics (Berlin), 2007-07, Vol.469 (2), p.687-706

2007

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The asteroseismic surface effect from a grid of 3D convection simulations – I. Frequency shifts from convective expansion of stellar atmospheres

Monthly notices of the Royal Astronomical Society. Letters, 2017-03, Vol.466 (1), p.L43-L47

2017

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ON THE AMPLITUDE OF CONVECTIVE VELOCITIES IN THE DEEP SOLAR INTERIOR

The Astrophysical journal, 2012-10, Vol.757 (2), p.1-14

2012

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An extended and refined grid of 3D STAGGER model atmospheres: Processed snapshots for stellar spectroscopy

Astronomy and astrophysics (Berlin), 2024-08, Vol.688, p.A212

2024

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Does the Scaling Relation Depend on Metallicity? Insights from 3D Convection Simulations

The Astrophysical journal, 2024-01, Vol.962 (2), p.118

2024

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CALIBRATING CONVECTIVE PROPERTIES OF SOLAR-LIKE STARS IN THE KEPLER FIELD OF VIEW

Astrophysical journal. Letters, 2012-08, Vol.755 (1), p.1-7

2012

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ON THE AMPLITUDE OF CONVECTIVE VELOCITIES IN THE DEEP SOLAR INTERIOR

The Astrophysical journal, 2012, Vol.755 (2)

2012

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The elemental composition of the Sun

Astronomy and astrophysics (Berlin), 2015-01, Vol.573

2015

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ON THE AMPLITUDE OF CONVECTIVE VELOCITIES IN THE DEEP SOLAR INTERIOR

The Astrophysical journal, 2012-10, Vol.757 (2), p.1-14

2012

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Using simulations of solar surface convection as boundary conditions on global simulations

Proceedings of the International Astronomical Union, 2010-06, Vol.6 (S271), p.403-404

2010

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The Chemical Compositions of the Extreme Halo Stars HE 0107-5240 and HE 1327-2326 Inferred from Three-dimensional Hydrodynamical Model Atmospheres

The Astrophysical journal, 2006, Vol.664 (2), p.L121

2006

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Isochrone fitting of the open cluster M67 in the era of Gaia and improved model physics

A GRID OF THREE-DIMENSIONAL STELLAR ATMOSPHERE MODELS OF SOLAR METALLICITY. I. GENERAL PROPERTIES, GRANULATION, AND ATMOSPHERIC EXPANSION

The Stagger Code for Accurate and Efficient, Radiation-coupled Magnetohydrodynamic Simulations

Does the νmax Scaling Relation Depend on Metallicity? Insights from 3D Convection Simulations

An opaque Sun? The potential for future, higher opacities to solve the solar abundance problem

The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission

Improving 1D Stellar Models with 3D Atmospheres

ON THE AMPLITUDE OF CONVECTIVE VELOCITIES IN THE DEEP SOLAR INTERIOR

Modeling the Near-Surface Shear Layer: Diffusion Schemes Studied With CSS

The Surface of Stellar Models - Now with more 3D simulations

The elemental composition of the Sun: I. The intermediate mass elements Na to Ca

Improvements to stellar structure models, based on a grid of 3D convection simulations – II. Calibrating the mixing-length formulation

The Mass Mixing Length in Convective Stellar Envelopes

Improvements to stellar structure models, based on a grid of 3D convection simulations – I. T(τ) relations

Three-dimensional hydrodynamical simulations of surface convection in red giant stars : Impact on spectral line formation and abundance analysis

The asteroseismic surface effect from a grid of 3D convection simulations – I. Frequency shifts from convective expansion of stellar atmospheres

ON THE AMPLITUDE OF CONVECTIVE VELOCITIES IN THE DEEP SOLAR INTERIOR

An extended and refined grid of 3D STAGGER model atmospheres: Processed snapshots for stellar spectroscopy

Does the Scaling Relation Depend on Metallicity? Insights from 3D Convection Simulations

CALIBRATING CONVECTIVE PROPERTIES OF SOLAR-LIKE STARS IN THE KEPLER FIELD OF VIEW

ON THE AMPLITUDE OF CONVECTIVE VELOCITIES IN THE DEEP SOLAR INTERIOR

The elemental composition of the Sun

ON THE AMPLITUDE OF CONVECTIVE VELOCITIES IN THE DEEP SOLAR INTERIOR

Using simulations of solar surface convection as boundary conditions on global simulations

The Chemical Compositions of the Extreme Halo Stars HE 0107-5240 and HE 1327-2326 Inferred from Three-dimensional Hydrodynamical Model Atmospheres

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