Short-term variability and mass loss in Be stars - IV. Two groups of closely spaced, approximately equidistant frequencies in three decades of space photometry of ν Puppis (B7-8 IIIe)

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Fig. 2.

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A 10-d stretch (in 2017) of observations of ν Pup with BRITE satellites BLb (blue filled triangles), BHr (red asterisks), and BTr (red crosses). The zeropoints of the magnitude scale are arbitrary. Black dots represent a sine fit to the BHr data. The deviation from sinusoidality is most clearly seen in the BHr data.

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