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To progress in our understanding of cool stars is instrumental to have access to UV (mid-high resolution) spectroscopy. In fact, the UV range supplies a richness of experimental data which is unmatched by any other spectral domain for the study [...]texto impreso
The International Ultraviolet Explorer (IUE) has been contemporary to the rapid development of the research on star formation. The IUE has contributed significantly to the understanding of the atmospheres of the T Tauri stars (TTSs) as well as t[...]texto impreso
We present a study of the UV emission lines fluxes of the T Tauri stars (TTS). We have used for this purpose the final IUE sample of TTS which includes 33 TTS with good spectra in whole IUE range. We have derived the lines fluxes and compared th[...]
