Issue |
A&A
Volume 503, Number 3, September I 2009
|
|
---|---|---|
Page(s) | 945 - 962 | |
Section | Stellar atmospheres | |
DOI | https://doi.org/10.1051/0004-6361/200811561 | |
Published online | 02 July 2009 |
Online Material
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Figure 8:
Same as Fig. 2, but also for H |
Open with DEXTER |
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Figure 9: Same as Fig. 8, but for HD 145788. |
Open with DEXTER |
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Figure 10:
Same as Fig. 8, but for |
Open with DEXTER |
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Figure 11:
Comparison between LLMODELS theoretical fluxes calculated with the
fundamental parameters and abundances derived for HD 145788, taking into
account a reddening of
E(B-V)=0.20 (full black line) and without taking
into account reddening (dashed black line), with IUE calibrated fluxes
(full blue line), Johnson UBV photometry (green squares), Geneva photometry (red
circles) and 2MASS photmetry (violet triangles). The model fluxes were
convolved to have approximately the same spectral resolution of the IUE fluxes
( R |
Open with DEXTER |
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Figure 12:
Comparison between the observed spectrum of the He I
line at
|
Open with DEXTER |
Table 6: Comparison of the derived abundances with previous determinations for 21 Peg.
Table 7:
Comparison of the derived abundances with previous dterminations for Cet.
Table 8: A collection of the experimental and theoretical transition probabilities and Stark widths for the observed Si II lines. Errors are given in parenthesis.
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