Fig. 11.
Doppler velocities at different orbital phases of Lyα lines and He-like triplets of S, Si, Mg, and Ne from Schulz et al. (2002) (blue) and Goldstein et al. (2004) (orange), from Grinberg et al. (2017) (green), and from the present work (red). Different symbols stand for different ionisation stages. The solid and dashed lines represent the radial velocities of the NS and of the companion star, respectively.
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