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Fig. 2


20092010 Brγ (black) and Hα (blue) time series of Rigel. The Brγ spectra are shown as the difference to an artificially created photospheric spectrum shown at MJD 55 130 (red). For Hα only the spectra taken closest in time to the Brγ spectra are shown. The normalised flux scale for Brγ is enlarged by a factor of two relative to the one of Hα to match the strength of profile variability of the two lines. The strong telluric water absorption line at − 400km s-1 is not resolved and provides an estimate of the spectral resolution of the AMBER spectra around Brγ. The complete 2009 time series are shown in Figs. C.1 and C.2.

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