X Tri

Mezzetti1980 - Mezzetti1980B (Johnson B)

The B & V light curves given are from Buzkurt et al. (1976). The radial velocity curve is from Struve (1946). The solutions presented are from Mezzetti et al. (1980). The solutions were modified by forcing the cooler star to exactly fit its inner Roche surface, and its temperature was increased from 4810 K to 5100 K to better fit the light curves. The geometrical parameters were taken from Mezzetti et al’s (1980) fit to the V light curve.