Fig. 1
Swift/XRT spectra of the WD symbiotics with newly discovered X-ray emission together with their X-ray spectral types: NQ Gem, UV Aur, ZZ CMi, ER Del, Hen 3-461, CD-28 3719, StHα 32, BI Cru, V347 Nor, and SWIFT J171951.7-300206. The full line shows the best-fit model described in Sect. 3, while the dotted line shows the contribution of the individual spectral components in the case of multi-component models. The X-ray spectral classification for each source is included between parentheses in each panel and is listed in Table 4.
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