V752 Cen
Barone1993 - Barone1993U (Johnson U)
The solutions presented here are from Barone et al. (1993). The omega potentials given in Table 3 of that paper do not fit the light curves at all, nor do they represent the fillout factor given in that same table. Assuming that their fillout factor of 0.087 is what they intended, these models were calculated with omega potentials of 6.7601. 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).