Accretion dynamics in the classical T Tauri star V2129 Ophiuchi
S. H. P. AlencarDepartamento de Física – ICEx – UFMG, Av. Antônio Carlos 6627, 30270-901 Belo Horizonte, MG, BrazilJ. BouvierUJF-Grenoble 1 / CNRS-INSU, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) UMR 5274, 38041 Grenoble, FranceF. M. WalterDepartment of Physics and Astronomy, Stony Brook University, Stony Brook, NY, 11794-3800, USAC. DougadosUJF-Grenoble 1 / CNRS-INSU, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) UMR 5274, 38041 Grenoble, FranceJ.‐F. DonatiIRAP-UMR 5277, CNRS and Univ. de Toulouse, 14 Av. E. Belin, 31400 Toulouse, FranceRyuichi KurosawaDepartment of Astronomy, Cornell University, Space Sciences Building, Ithaca, NY 14853-6801, USAM. M. RomanovaDepartment of Astronomy, Cornell University, Space Sciences Building, Ithaca, NY 14853-6801, USAX. BonfılsUJF-Grenoble 1 / CNRS-INSU, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) UMR 5274, 38041 Grenoble, FranceG. H. R. A. LimaDepartamento de Física – ICEx – UFMG, Av. Antônio Carlos 6627, 30270-901 Belo Horizonte, MG, BrazilS. MassaroINAF – Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134 Palermo, ItalyM. IbrahimovUlugh Beg Astronomical Institute of the Uzbek Academy of Sciences, Astronomicheskaya 33, 700052 Tashkent, UzbekistanE. PorettiINAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (LC), Italy
ABI
Abstract
Context. Classical T Tauri stars are variable objects on several timescales, but just a few of them have been studied in detail, with different observational techniques and over many rotational cycles to enable the analysis of the stellar and circumstellar variations on rotational timescales.
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