%0 Conference Proceedings
%T The evolution of surface magnetic fields in young solar-type stars
%+ Institut de recherche en astrophysique et planétologie (IRAP)
%+ Institut de Planétologie et d'Astrophysique de Grenoble (IPAG )
%+ Laboratoire Univers et Particules de Montpellier (LUPM)
%+ Institut für Astrophysik [Göttingen]
%A Folsom, C. P.
%A Petit, P.
%A Bouvier, J.
%A Donati, J. -F.
%A Morin, Julien
%Z To appear in the proceedings of IAU symposium 302: Magnetic fields throughout stellar evolution. 2 pages, 3 figures
%< avec comité de lecture
%Z LUPM:13-056
%( Magnetic fields throughout stellar evolution
%B IAU symposium 302: Magnetic fields throughout stellar evolution
%C Biarritz, France
%V 302
%P 110
%8 2013-08-25
%D 2013
%Z 1310.2073
%R 10.1017/S1743921314001835
%Z Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Conference papers
%X The surface rotation rates of young solar-type stars decrease rapidly with age from the end of the pre-main sequence though the early main sequence. This suggests that there is also an important change in the dynamos operating in these stars, which should be observable in their surface magnetic fields. Here we present early results in a study aimed at observing the evolution of these magnetic fields through this critical time period. We are observing stars in open clusters and stellar associations to provide precise ages, and using Zeeman Doppler Imaging to characterize the complex magnetic fields. Presented here are results for six stars, three in the in the beta Pic association (~10 Myr old) and three in the AB Dor association (~100 Myr old).
%G English
%L hal-01770050
%U https://hal.science/hal-01770050
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