All Tables

Table 1: VLTI/MIDI observations of S Ori.
Table 2: Properties of the MIDI calibration stars used.
Table 3: Fit results of our MIDI measurements of S Ori.
Table 4: Reduced $\chi ^2_\nu$ values obtained for our grid of overall models.
Table 5: VLBA observations of S Ori.
Table 6: Results from our VLBA observations of the v=1, 43.1 GHz and v=2, 42.8 GHz SiO maser transition toward S Ori.
Table 7: Overview of the photometric and spatial parameters of S Ori as a function of stellar phase, derived from both our VLTI and VLBA observations.