V752 Cen
Leung1976 - Leung1976B (Johnson B)
The models presented are those of Leung (1976). The temperature of star 2 was increased slightly from 6234 K to 6300 K to better fit the light curves. Leung (1976) used radiative values for albedo and gravity brightening, whereas for stars of these temperatures the convective values should probably be used (as done in Barone et al. (1993)). The UBV observations of Sisteró & Castore de Sisteró (1973) that were analyzed show asymmetries in the quadratures most likely due to starspots that were not modeled. The radial velocity observations are from Sisteró & Castore de Sisteró (1974).