Fig. C.1.
Time series analysis of optical emission lines of the V2129 Oph data from Alencar et al. (2012). Shown are bidimensional periodograms (left) and the corresponding line profiles (right). Left panels: the color range corresponds to the normalized power of the periodogram, and the horizontal solid line represents the rotation period of the star, P = 6.53 days. Right panels: different colors correspond to different rotation cycles.
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