Online material
Appendix A: Best fits
In this Appendix we present our best-fit models to the optical and UV spectra for the eight stars in our sample. The wavelength range between 1200 and 1225 Å was not used in the spectral analysis since it suffers from a strong interstellar Lyman absorption. Nevertheless, we take this interstellar absorption into account by adding the effects of a representative hydrogen column density to our synthetic spectra in our final plots.
 |
Fig. A.1
Best-fit model for HD 190429A (red line) compared to FUSE and IUE spectra (black line). |
| Open with DEXTER | |
 |
Fig. A.2
Best-fit model for HD 190429A (red line) compared to the ELODIE spectrum (black line). |
| Open with DEXTER | |
 |
Fig. A.3
Best-fit model for HD 66811 (red line) compared to Copernicus and IUE spectra (black line). |
| Open with DEXTER | |
 |
Fig. A.4
Best-fit model for HD 66811 (red line) compared to the FEROS spectrum (black line). |
| Open with DEXTER | |
 |
Fig. A.5
Best-fit model for HD 16691 (red line) compared to FUSE and IUE spectra (black line). |
| Open with DEXTER | |
 |
Fig. A.6
Best-fit model for HD 16691 (red line) compared to the ELODIE spectrum (black line). |
| Open with DEXTER | |
 |
Fig. A.7
Best-fit model for HD 15570 (red line) compared to FUSE and IUE spectra (black line). |
| Open with DEXTER | |
 |
Fig. A.8
Best-fit model for HD 15570 (red line) compared to the ELODIE spectrum (black line). |
| Open with DEXTER | |
 |
Fig. A.9
Best-fit model for HD 14947 (red line) compared to FUSE and IUE spectra (black line). |
| Open with DEXTER | |
 |
Fig. A.10
Best-fit model for HD 14947 (red line) compared to the ELODIE spectrum (black line). |
| Open with DEXTER | |
 |
Fig. A.11
Best-fit model for HD 210839 (red line) compared to FUSE and IUE spectra (black line). |
| Open with DEXTER | |
 |
Fig. A.12
Best-fit model for HD 210839 (red line) compared to the NARVAL spectrum (black line). |
| Open with DEXTER | |
 |
Fig. A.13
Best-fit model for HD 163758 (red line) compared to FUSE and IUE spectra (black line). |
| Open with DEXTER | |
 |
Fig. A.14
Best-fit model for HD 163758 (red line) compared to the UVES spectrum (black line). |
| Open with DEXTER | |
 |
Fig. A.15
Best-fit model for HD 192639 (red line) compared to FUSE and IUE spectra (black line). |
| Open with DEXTER | |
 |
Fig. A.16
Best-fit model for HD 192639 (red line) compared to the ELODIE spectrum (black line). |
| Open with DEXTER | |
© ESO, 2012