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Fig. 3.

image

Example spectrum of the central star of PN G283.7−05.1 (in black), taken at an orbital phase of roughly 0.26. The spectrum highlights the prominent absorption spectrum of the primary as well as the extremely weak nature of the irradiated emission line complex. A TMAP synthetic spectrum with Teff and surface gravity roughly consistent with the PHOEBE2 model is underlaid in red.

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