Fig. 5.
Closeup of the profiles near eclipse in trailed spectra of three of the lines from the Magellan data: HeII 4541 (top left), HeII 4859 (top right), HeII 5411 (bottom left), and the average of these three lines (bottom right). The eclipse is indicated by the white lines and is visible as a darkening around phase 0.0 that slopes upwards from the blue- to the redshifted sides of the lines.
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