X-ray spectra of the symbiotic stars: (a) BD Cam using Swift data, (b) V1261 Ori using the tbabs × mkcflow model, and (c) V1261 Ori using the tbabs × compTT model, (d) NQ Gem, and (e) CD −27 8661. These data were obtained with XMM-Newton where the black color is EPIC-pn, the red is EPIC-MOS 1, and the green is EPIC-MOS 2. The solid lines show the best-fit models given in Table 3. The dotted lines show the contribution of the individual spectral components in the case of multicomponent models.