Fig. 2.
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Orbital solutions of all the newly classified SB2s in our sample. The dashed red line represents the RV curve of the secondary star. We stress that the RVs of the secondaries are not fitted individually from the spectra, but are forced to vary in anti-phase with the primary and with the semi-amplitude derived through spectral disentangling (Sect. 3.2). (a) HD 29763. (b) HD 30836. (c) HD 52533. (d) HD 57236. (e) HD 91824. (f) HD 93028. (g) HD 152405. (h) HD 152723. (i) HD 163892. (j) HD 164438. (k) HD 164536. (l) HD 167263. (m) HD 167264. (n) HD 192001. (o) HD 199579. (p) Schulte 11. (q) V747 Cep.
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