ζ Aurigue type systems are of great interest in the
field of astrophysics, since they are binary systems
"rare" whose components are: a giant or
cold supergiant (of approximately R = 200R and
M = 8.3M) and a hot main sequence star (of about R = 4R and M = 5.6M).
[Kopal,2012]. In this research work it is believed
a complete database, as well as the representation
graph of their changes in the different phases they present. These data will serve as support for future research in the field of stellar physics.