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Appendix A: Spectral fits
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Fig. A.1
Best fit from PoWR modeling (thick red solid lines) to the observed HD 66811 spectra (thin blue solid lines), together with the calculated P v line profile from 3D Monte-Carlo code (black dotted line). Blue labels with numbers in the upper panels are UBVJHK magnitudes. |
| Open with DEXTER | |
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Fig. A.2
Same as Fig. A.1, but for HD 15570. |
| Open with DEXTER | |
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Fig. A.3
Same as Fig. A.1, but for HD 14947. |
| Open with DEXTER | |
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Fig. A.4
Same as Fig. A.1, but for HD 210839. |
| Open with DEXTER | |
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Fig. A.5
Same as Fig. A.1, but for HD 192639. |
| Open with DEXTER | |
© ESO, 2013