Modeling the Complete Lightcurve of ω CMa

We have used the radiative transfer code HDUST to analyze and interpret the long-term photometric behavior of the Be star ω CMa, considering four complete cycles of disk formation and dissipation. This is the first time in which a full lightcurve of a Be star was investigated and modeled including both disk build-up and dissipation phases. Based on the quite good fit of the observed data we were able to derive the history of stellar mass decretion rates (including long- and short-term changes) during the disk formation and dissipation phases in all four cycles.