Fig. 4.
Phase-folded RVs of the hot (blue) and cool (red) components of the central star system of PN G283.7−05.1, overlaid on the best-fitting PHOEBE2 model RV curves. The centre-of-mass RV curve of the secondary is shown as the dotted grey line, while the RV of its innermost point (i.e. the most highly irradiated part of the stellar surface) is shown as the dashed grey line.
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