Fig. 14
Theoretical line profiles for m1 with R1 = 7.6R⊙ and 8.4 R⊙ (dash) in the orbital phase intervals 0.24–0.44 and 0.74–0.94 for ωper = 233°. The orbital phases run from bottom to top, as indicated. Note that the most significant differences between the profiles of different radii is in the “bumps” as the star approaches periastron (right).
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