All Tables

• Table 1: AMBER observation log from 31 May 2004 (UT).
• Table 2: Calibrated visibilities obtained with different algorithms and data selection.
• Table 3: The best-fit accretion disk model parameters found by simultaneous fitting of SED and visibilities.
• Table 4: The best-fit model parameters for the outflowing wind model. Most parameters are self-explanatory (see Appendix A for details). C₁ is the ratio between the polar and equatorial mass flux; m₁ is the exponent of the mass flux law as a function of latitude; m₂ is the exponent of the latitude dependent terminal velocity law.