Fig. 4
Model spectra for He I, generated every 20° of orbital phase. The lowest spectrum is for orbital phase 0; successive spectra are successively displaced upwards by 1. The top spectrum is for 340° and the model spectrum shown in Fig. 2 immediately precedes it. The model spectrum shown in Fig. 3 is also included. This compilation can be compared with the observed spectra in Fig. 2 of Blundell & Schmidtobreick (2006).
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