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- W1765562291 abstract "We have used the radiative transfer code HDUST to analyze and interpret the long-term photometric behavior of the Be star omega 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." @default.
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- W1765562291 date "2015-06-29" @default.
- W1765562291 modified "2023-09-27" @default.
- W1765562291 title "Modeling the Complete Lightcurve of omega CMa" @default.
- W1765562291 hasPublicationYear "2015" @default.
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