Observational Contrains on Collimation Mechanisms in RU Lupi
A large campaign of multifrequency observations of extreme T Tauri star RU Lupi was performed from 1983 to 1988. We present here main observational results of the campaign and their preliminary interpretation in terms of disk accretion onto an young star with moderately strong global magnetic field.
KeywordsDisk Accretion Young Star Balmer Line Bolometric Luminosity Accretion Column
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- Giovannelli F., Vittone A.A., Rossi C., Nastari I., Bisnovatyi-Kogan G.S., Golynskaya I.M., Kurt V.G., Mizyakina T.A., Shafer E.Y., Shamolin V.M., ShefferE.K., Smirnoff A.S., Lamzin S.A., Larionov M.G., Sidorenko V.N.: 1986, in New Insight in Astrophysics, ESA SP-263, 95Google Scholar
- Zeldovich Ya.B., Rayzer Yu.P.: 1966, Physics of shock waves and high temperature hydrodynamics phenomena, Academic PressGoogle Scholar