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Communication Dans Un Congrès Année : 2019

Fossil magnetic fields in intermediate-mass and massive stars

Résumé

A small fraction of the population of intermediate-mass and massive stars host strong and stable magnetic fields organised on large scales. These fields are believed to be remnants of star formation. It is however not clear how such fossil fields have been shaped during their formation and subsequent evolution. We report recent and ongoing studies on the magnetic properties of pre-main sequence stars and main sequence binaries, allowing us to make progress in this field.

Dates et versions

hal-02323240 , version 1 (21-10-2019)

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E. Alecian, F. Villebrun, J. Grunhut, G. Hussain, Coralie Neiner, et al.. Fossil magnetic fields in intermediate-mass and massive stars. Astro Fluid: An International Conference in Memory of Professor Jean-Paul Zahn's Great Scientific Achievements, 2016, Paris, France. pp.345-355, ⟨10.1051/eas/1982030⟩. ⟨hal-02323240⟩
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