Abstract
SU Aur is a G2 classical TTauri star. The Balmer lines in this star show very large intensity fluctuations, and a persistent pattern of simultaneous gas inflow and outflow around the star has been reported (Petrov et al., 1996).
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Giampapa M.S. et al. (1993), ApJ, 89, 321
Johns CM. & Basri G. (1995), ApJ, 449, 341
Petrov P.P. et al. (1996), A&A, 314, 821
Unruh Y.C. et al. (1997), The 10th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, ed. R.A. Donahue & J.A. Bookbinder, in press
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© 1999 Springer Science+Business Media Dordrecht
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Oliveira, J.M., Unruh, Y.C., Foing, B.H. (1999). Balmer Line Profiles Variations in SU Aurigae from the Musicos 96 Multi-Site Campaign. In: Lago, M.T.V.T., Blanchard, A. (eds) The Non-Sleeping Universe. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4497-1_34
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DOI: https://doi.org/10.1007/978-94-011-4497-1_34
Publisher Name: Springer, Dordrecht
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