AE Cas
Bradstreet2005 - Bradstreet2005B (Johnson B)
The UBV light curves are from Srivastava & Kandpal (1984). The model solution is a rough estimate made by me based upon their solution since Srivastava & Kandpal (1984) used Kopal’s frequency domain method and do not give parameters like mass ratio, temperatures, etc. The light curves contain significant noise. The temperature difference required for the two stars is somewhat greater than the spectral classes suggested by Srivastava & Kandpal.