Magnetic fields of intermediate-mass T Tauri stars

Context. The origin of the fossil magnetic fields detected in 5 to 10% of intermediate-mass main sequence stars is still highly debated. Aims. We want to bring observational constraints to a large population of intermediate-mass pre-main sequence (PMS) stars in order to test the theory that convecti...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2019-02, Vol.622
Hauptverfasser:	Villebrun, F., Alecian, E., Hussain, G., Bouvier, J., Folsom, C. P., Lebreton, Y., Amard, L., Charbonnel, C., Gallet, F., Haemmerlé, L., Böhm, T., Johns-Krull, C., Kochukhov, O., Marsden, S. C., Morin, J., Petit, P.
Format:	Artikel
Sprache:	eng
Schlagworte:	Detection limits Dipoles Envelopes Herbig Ae/Be Magnetic fields Magnetic properties Magnetic stars Main sequence stars Mathematical models Parameters Photometry Pre-main sequence stars stars: activity stars: fundamental parameters stars: magnetic field stars: pre-main sequence stars: variables: T Tauri Stellar evolution Stellar magnetic fields Stellar mass T Tauri stars
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