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Fig. 7.

image

Available ionization energy of Model O.50 in the orbital plane at the beginning of the simulation, after one and after four orbits. The white and light blue lines represent projections of the photosphere along the axes (i.e., they outline the opaque region). The red, green and dark blue contours enclose regions with ionization fractions of H, HeI, and HeII larger than 0.2, respectively.

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