Issue |
A&A
Volume 510, February 2010
|
|
---|---|---|
Article Number | A22 | |
Number of page(s) | 21 | |
Section | Stellar atmospheres | |
DOI | https://doi.org/10.1051/0004-6361/200913120 | |
Published online | 02 February 2010 |
Online Material
Table 5: List of log gf values for the Si II-IV lines considered in this study (from Atomic Line List v2.05). For the O II lines we refer to Simón-Díaz et al. (2006).
Table 6: Results from the abundance analysis of HD 36512 (B0 V).
Table 7: Results from the abundance analysis of HD 37020 (B0.5 V).
Table 8: Results from the abundance analysis of HD 36960 (B0.5 V).
Table 9: Results from the abundance analysis of HD 37042 (B0.7 V).
Table 10: Results from the abundance analysis of HD 36591 (B1 V).
Table 11: Results from the abundance analysis of HD 36959 (B1 V).
Table 12: Results from the abundance analysis of HD 37744 (B1.5 V).
Table 13: Results from the abundance analysis of HD 35299 (B1.5 V).
Table 14: Results from the abundance analysis of HD 36285 (B2 V).
Table 15: Results from the abundance analysis of HD 35039 (B2 V).
Table 16: Results from the abundance analysis of HD 36629 (B2 V).
Table 17: Results from the abundance analysis of HD 36430 (B2 V).
Table 18: Results from the abundance analysis of HD 35912 (B2 V).
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Figure 8: The complete atlas of FIES@ NOT spectra (part 1 of 3). The Si II-IV and O II lines used for the abundance analysis are indicated as solid and dashed vertical lines, respectively. |
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Figure 8: continued. |
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Figure 8: continued. |
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