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Stellar magnetohydrodynamics

All stars rotate and many exhibit complex surface magnetic fields and activity. Coupled with the presence of turbulent convective envelopes...

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Stellar models and evolution

With sufficiently good data, the asteroseismic determination of mass and radius can be essentially independent of stellar models. For other...

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Stellar parameters as key to exoplanet parameter accuracy

The main focus of the asteroseismology programme of PLATO will be to support exoplanet science by providing: stellar masses with...

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Probing stellar structure and evolution by asteroseismology

Asteroseismology is the study of the global oscillations of stars (see Aerts et al. 2010, Chaplin & Miglio 2013). These oscillations...

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