All Tables

Table 1: Characteristics of the sample of T Tauri stars, sorted by H $\alpha$ emission, for which high resolution X-ray spectra have been analyzed. In the case of resolved multiple systems the stellar mass, spectral type, and bolometric luminosity refer to the component responsible for the X-ray emission.
Table 2: Log of the XMM observation of TWA 5 (Rev. 565, ObsId 0112880101).
Table 3: TWA 5 best fit paramenters.
Table 4: Total counts (lines + continuum) in the interval 10-30 Å band vs. Fe abundance.
Table A.1: Strongest RGS lines of TWA 5.