| Issue |
A&A
Volume 546, October 2012
|
|
|---|---|---|
| Article Number | A55 | |
| Number of page(s) | 13 | |
| Section | Stellar atmospheres | |
| DOI | https://doi.org/10.1051/0004-6361/201220014 | |
| Published online | 04 October 2012 | |
Online material
 |
Fig. 4
He I / He II, C III / C IV, and O IV / O V ionization equilibria in our Teff = 70 kK model compared with FUSE, GHRS (smoothed with a low-pass filter (m = 15, n = 4) for clarity, Savitzky & Golay 1964), and UVES observations. Wavelength and flux scales are indicated by bars. The model spectrum is convolved with a Gaussian to match the respective instrument’s resolution. Unidentified lines in the model stem from Ca-Ni. |
| Open with DEXTER | |
 |
Fig. 5
Same as Fig. 4 for Teff = 65 kK. |
| Open with DEXTER | |
 |
Fig. 6
Same as Fig. 3 for Teff = 65 kK. |
| Open with DEXTER | |
Energy levels of Ge V (in cm-1). The first three LS-components are given when they are over 5%.
Energy levels of Ge VI (in cm-1). The first three LS-components are given when they are over 5%.
© ESO, 2012
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