Magnetospheric accretion-ejection processes in the classical T Tauri star AA Tauri
J. BouvierLaboratoire d'Astrophysique de Grenoble, Université Joseph-Fourier, BP 53, 38041 Grenoble Cedex 9, France e-mail: [email protected]S. H. P. AlencarDepartamento de Física, ICEx-UFMG, CP. 702, Belo Horizonte, MG, 30123-970, BrazilT. BoutelierLaboratoire d'Astrophysique de Grenoble, Université Joseph-Fourier, BP 53, 38041 Grenoble Cedex 9, France e-mail: [email protected]C. DougadosLaboratoire d'Astrophysique de Grenoble, Université Joseph-Fourier, BP 53, 38041 Grenoble Cedex 9, France e-mail: [email protected]Z. BalogSteward Observatory, University of Arizona, 933 N. Cherry Av., Tucson AZ 85721, USAK. N. GrankinUlugh Beg Astronomical Institute of the Uzbek Academy of Sciences, Astronomicheskaya 33, 700052 Tashkent, UzbekistanS. T. HodgkinInstitute of Astronomy, Madingley Road, Cambridge CB3 0HA, UKM. IbrahimovUlugh Beg Astronomical Institute of the Uzbek Academy of Sciences, Astronomicheskaya 33, 700052 Tashkent, UzbekistanM. KunKonkoly Observatory, 1525 Budapest PO Box 67, HungaryT. Yu. MagakianV.A. Ambartsumyan Byurakan Astrophysical Observatory, ArmeniaC. PinteLaboratoire d'Astrophysique de Grenoble, Université Joseph-Fourier, BP 53, 38041 Grenoble Cedex 9, France e-mail: [email protected]
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Context.Accretion and ejection are complex and related processes that vary on various timescales in young stars.
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