All Tables

• Table 1: Top: V magnitudes, parallaxes and absolute magnitudes of V390 Aurigae. Middle: spectral type, color indices and effective temperature. Bottom: estimated stellar parameters of V390 Aurigae.
• Table 2: V390 Aurigae observation log during XMM-Newton revolution 135 and 232.
• Table 3: X-ray luminosities (corrected for interstellar absorption) of V390 Aurigae in the 0.3-2 keV and 2-10 keV bands. The percentage contribution in luminosity of hot plasmas (kT>1 keV) is indicated between brackets.
• Table 4: Best fit parameters to EPIC data using a two component MEKAL model (Mewe et al. 1985) with variable abundance and a variable hydrogen column density.
• Table 5: Measured positions and fluxes of the strongest lines in the RGS spectra of V390 Aurigae obtained during revolutions 135 and 232. The columns give the predicted line positions, the measured line positions during revolution 135, the measured line positions during revolution 232, the ion and line identifications, the temperatures of maximum line formation, the line fluxes measured during revolution 135 and the line fluxes measured during revolution 232.
• Table 6: Best fit parameters to RGS spectra in the 0.6-1.3 keV range recorded in revolutions 135 and 232 using a two component VMEKAL model. The temperature and metallicity of each component were frozen to the value derived from the analysis of EPIC data (see Table 4). The oxygen and neon abundances of the high temperature component were left free to vary.
• Table 7: Physical parameters of V390 Aurigae coronal loops.