The birth of Be star disks - I. From localized ejection to circularization

Open Access

Fig B.10.

Similar to Fig. B.8 for κ CMa. Outburst events are even less clearly delineated than in 25 Ori, but two sections of EW_V/EW_R measurements could be fit with Eq. 2. The full timeseries is not fit well with a single frequency (e.g., treating the full timeseries as one long “event”).

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