EDP Sciences
Free Access
Issue
A&A
Volume 544, August 2012
Article Number A67
Number of page(s) 30
Section Stellar atmospheres
DOI https://doi.org/10.1051/0004-6361/201118594
Published online 27 July 2012

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.

thumbnail Fig. A.1

Best-fit model for HD 190429A (red line) compared to FUSE and IUE spectra (black line).

Open with DEXTER

thumbnail Fig. A.2

Best-fit model for HD 190429A (red line) compared to the ELODIE spectrum (black line).

Open with DEXTER

thumbnail Fig. A.3

Best-fit model for HD 66811 (red line) compared to Copernicus and IUE spectra (black line).

Open with DEXTER

thumbnail Fig. A.4

Best-fit model for HD 66811 (red line) compared to the FEROS spectrum (black line).

Open with DEXTER

thumbnail Fig. A.5

Best-fit model for HD 16691 (red line) compared to FUSE and IUE spectra (black line).

Open with DEXTER

thumbnail Fig. A.6

Best-fit model for HD 16691 (red line) compared to the ELODIE spectrum (black line).

Open with DEXTER

thumbnail Fig. A.7

Best-fit model for HD 15570 (red line) compared to FUSE and IUE spectra (black line).

Open with DEXTER

thumbnail Fig. A.8

Best-fit model for HD 15570 (red line) compared to the ELODIE spectrum (black line).

Open with DEXTER

thumbnail Fig. A.9

Best-fit model for HD 14947 (red line) compared to FUSE and IUE spectra (black line).

Open with DEXTER

thumbnail Fig. A.10

Best-fit model for HD 14947 (red line) compared to the ELODIE spectrum (black line).

Open with DEXTER

thumbnail Fig. A.11

Best-fit model for HD 210839 (red line) compared to FUSE and IUE spectra (black line).

Open with DEXTER

thumbnail Fig. A.12

Best-fit model for HD 210839 (red line) compared to the NARVAL spectrum (black line).

Open with DEXTER

thumbnail Fig. A.13

Best-fit model for HD 163758 (red line) compared to FUSE and IUE spectra (black line).

Open with DEXTER

thumbnail Fig. A.14

Best-fit model for HD 163758 (red line) compared to the UVES spectrum (black line).

Open with DEXTER

thumbnail Fig. A.15

Best-fit model for HD 192639 (red line) compared to FUSE and IUE spectra (black line).

Open with DEXTER

thumbnail Fig. A.16

Best-fit model for HD 192639 (red line) compared to the ELODIE spectrum (black line).

Open with DEXTER


© ESO, 2012

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