Issue |
A&A
Volume 536, December 2011
|
|
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Article Number | A82 | |
Number of page(s) | 15 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/201116802 | |
Published online | 13 December 2011 |
Online material
Appendix A: Light curves and frequency spectra of B8/B9 stars observed with CoRoT
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Fig. A.1
Excerpt of the CoRoT light curve of HD 181440, showing multiperiodic variability (grey line shows a fit to the light curve, black dots represent to CoRoT data). |
Open with DEXTER |
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Fig. A.2
Frequency spectrum of the CoRoT light curve of HD 181440 above 0.1 d-1 (black). The significant frequencies and fitted amplitudes above 10 ppm are indicated in grey. |
Open with DEXTER |
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Fig. A.3
Excerpt of the CoRoT light curve of HD 182198, with only one clear clear frequency (grey line shows a fit to the light curve, black dots represent to CoRoT data). |
Open with DEXTER |
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Fig. A.4
Frequency spectrum of the CoRoT light curve of HD 182198 above 0.1 d-1 (black). The significant frequencies and fitted amplitudes above 10 ppm are indicated in grey. |
Open with DEXTER |
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Fig. A.5
Excerpt of the CoRoT light curve of HD 49677, with only one clear frequency detected (grey line shows a fit to the light curve, black dots represent to CoRoT data). |
Open with DEXTER |
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Fig. A.6
Frequency spectrum of the CoRoT light curve of HD 49677 above 0.1 d-1 (black). The significant frequencies with amplitudes above 10 ppm are indicated in grey. |
Open with DEXTER |
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Fig. A.7
Excerpt of the CoRoT light curve of HD 46179. No clear signs of variability are detected (grey line shows a fit to the light curve, black dots represent to CoRoT data). |
Open with DEXTER |
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Fig. A.8
Frequency spectrum of the CoRoT light curve of HD 46179 above 0.1 d-1 (black). The significant frequencies with amplitudes above 10 ppm are indicated in grey. |
Open with DEXTER |
© ESO, 2011
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