| Issue |
A&A
Volume 538, February 2012
|
|
|---|---|---|
| Article Number | A39 | |
| Number of page(s) | 19 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361/201117458 | |
| Published online | 30 January 2012 | |
Online material
Appendix A: Best fit to the observed spectra
Figures A.1 to A.4 show the observed spectra in black together with the best fit CMFGEN models in red.
 |
Fig. A.1
Best CMFGEN fits (red) of the optical spectra (black) of stars HD 46573 (top), HD 46485 (bottom). The models have the mass-loss rate that best reproduces the UV features. The unfitted feature around 4425 Å is a DIB. |
| Open with DEXTER | |
 |
Fig. A.2
Best CMFGEN fits (red) of the optical spectra (black) of stars HD 46056 (top), HD 46966 (bottom). The models have the mass-loss rate that best reproduces the UV features. The unfitted feature around 4425 Å is a DIB. |
| Open with DEXTER | |
 |
Fig. A.3
Best CMFGEN fits (red) of the optical spectra (black) of stars HD 46223 (top), HD 46202 (bottom). The models have the mass-loss rate that best reproduces the UV features. The unfitted feature around 4425 Å is a DIB. |
| Open with DEXTER | |
 |
Fig. A.4
Best CMFGEN fits (red) of the optical spectra (black) of the primary (top) and secondary (bottom) components of HD 46149. The models have the mass-loss rate that best reproduces the UV features. The unfitted feature around 4425 Å is a DIB. |
| Open with DEXTER | |
© ESO, 2012
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