Short-term variability and mass loss in Be stars - III. BRITE and SMEI satellite photometry of 28 Cygni

D. Baade; A. Pigulski; Th. Rivinius; A. C. Carciofi; D. Panoglou; M. R. Ghoreyshi; G. Handler; R. Kuschnig; A. F. J. Moffat; H. Pablo; A. Popowicz; G. A. Wade; W. W. Weiss; K. Zwintz

doi:10.1051/0004-6361/201731187

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Volume 610 (February 2018)

A&A, 610 (2018) A70

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Fig. 19

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Combination of 60 BeSS Hα profiles between mJD 589 and 733. The spectra were averaged over a window of 20 d stepped by 2 d. The spectral bin size is 0.1 Å. Only three spectra were obtained before mJD 633. The BRITE observations terminated on mJD 665.

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