Abstract
A large campaign of multifrequency observations of the extreme T Tauri star RU Lupi was performed from 1983 to 1988.
We present some observational results and a first attempt of their interpretation. The various phenomena observed in RU Lupi can be explained in term of a disk accretion onto an young star with a moderately strong global magnetic field. The role of axial rotation is also discussed.
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Giovannelli, F. et al. (1991). Multifrequency Monitoring of RU Lupi: Observational Results and a Model. In: Catalano, S., Stauffer, J.R. (eds) Angular Momentum Evolution of Young Stars. NATO ASI Series, vol 340. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-3580-1_9
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