Jon Sundqvist

Associate Professor

KU Leuven

Belgium

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About

Jon Sundqvist is an Associate Professor at KU Leuven, Belgium. His research focuses on radiation-magnetohydrodynamics, stellar atmosphere modeling, and the structure formation of O-type and Wolf-Rayet stars. He has contributed to significant advancements in the understanding of massive stars in low metallicity environments and has published extensively in these areas, utilizing advanced simulation techniques.

Articles (16)

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2025

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2021

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2021

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2021

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2021

Collaborators (6)

Roel Lefever

Heidelberg University

GERMANY

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rony keppens

Gewoon Hoogleraar (Full Professor). Division Chair from May 2009 till July 2019.

KU Leuven

BELGIUM

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Paul Crowther

Professor of Astrophysics

University of Sheffield

UNITED KINGDOM

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Hugues Sana

Professor

KU Leuven

BELGIUM

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Calum Hawcroft

Space Telescope Science Institute

UNITED STATES

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Joachim Puls

research scientist/lecturer Dr. Dr. habil.

Ludwig-Maximilians-Universität München

GERMANY

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Jon Sundqvist

Research Interests

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About

Articles (16)

Improving 1D stellar atmosphere models with insights from multi-dimensional simulations

Radiation-magnetohydrodynamics with MPI-AMRVAC using flux-limited diffusion

Structure formation in O-type stars and Wolf–Rayet stars

Suppression of photospheric velocity fluctuations in strongly magnetic O stars in radiation-magnetohydrodynamic simulations

2D unified atmosphere and wind simulations of O-type stars

X-Shooting ULLYSES: Massive Stars at low metallicity

X-Shooting ULLYSES: Massive stars at low metallicity

Method and new tabulations for flux-weighted line opacity and radiation line force in supersonic media

The R136 star cluster dissected with Hubble Space Telescope/STIS

First 3D radiation-hydrodynamic simulations of Wolf-Rayet winds

New empirical mass-loss rates and clumping properties of massive stars

Radiation-hydrodynamics with MPI-AMRVAC

Empirical mass-loss rates and clumping properties of Galactic early-type O supergiants

Weakening the wind with ULLYSES: Examining the Bi-Stability Jump

Dynamically inflated wind models of classical Wolf-Rayet stars

Analytic, dust-independent mass-loss rates for red supergiant winds initiated by turbulent pressure

Collaborators (6)

Roel Lefever

rony keppens

Paul Crowther

Hugues Sana

Calum Hawcroft

Joachim Puls

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