Can we predict the magnetic properties of PMS stars from their H-R diagram location? Auteur(s): Gregory S. G., Donati J. -F., Morin J., Hussain G. A. J., Mayne N. J., Hillenbrand L. A., Jardine M.
Conference: IAUS 302: Magnetic Fields throughout Stellar Evolution (Biarritz, FR, 2013-08-25) Ref HAL: hal-01770047_v1 Ref Arxiv: 1309.7556 DOI: 10.1017/S1743921314001677 Ref. & Cit.: NASA ADS Exporter : BibTex | endNote Commentaires: Proceedings of IAUS 302: magnetic fields throughout stellar evolution, Biarritz, France, August 2013. CUP, in press |