Abstract
The T Tauri stars (TTS) are low-mass, pre-main-sequence stars. It is well known that the UV emission lines fluxes of the TTS are significantly higher than the observed in late-type main sequence stars. In this work we make use of the IUE Final Archive data to study this problem.
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Ayres T.R. Fleming T. A. Simon T. et al. 1995 ApJS 96. 22
Gómez de Castro, A.I., Franqueira, M. (1988) Access Guide n.8, SP-ESA, 1205. ESA Publication Division, ESTEC, Noordwijk, The Neetherlands.
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© 1999 Springer Science+Business Media Dordrecht
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Huélamo, N., Gómez De Castro, A.I., Franqueira, M. (1999). X Rays and UV Emission Lines in T Tauri Stars. 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_29
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DOI: https://doi.org/10.1007/978-94-011-4497-1_29
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-5923-7
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