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Results of the ROTOR-program

K. N. GrankinAstronomical Institute of the Uzbek Academy of Sciences, 700052 Tashkent, UzbekistanJ. BouvierLaboratoire d'Astrophysique, Observatoire de Grenoble, Universit Joseph Fourier, BP 53, 38041 Grenoble Cedex 9, FranceW. HerbstAstronomy Department, Wesleyan University, Middletown, CT 06459, USA e-mail: [email protected]S. MelnikovAstronomical Institute of the Uzbek Academy of Sciences, 700052 Tashkent, Uzbekistan
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Abstract

Context.T Tauri stars exhibit variability on all timescales, whose origin is still debated. On WTTS the variability is fairly simple and attributed to long-lived, ubiquitous cool spots.

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