Issue |
A&A
Volume 528, April 2011
|
|
---|---|---|
Article Number | A21 | |
Number of page(s) | 15 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/201016227 | |
Published online | 21 February 2011 |
Online material
Journal of spectroscopic observations at Cerro Armazones Observatory.
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Fig. 5
Rotational profile fit to all broadening functions outside eclipses. The panels give the orbital phase and the heliocentric Julian date (with 2 400 000 subtracted). The profile of the primary component (Aa) is plotted in black, the profile of the secondary component (Ab) in green, and the combined profile in blue. |
Open with DEXTER |
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Fig. 5
continued. |
Open with DEXTER |
![]() |
Fig. 5
continued. |
Open with DEXTER |
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Fig. 6
The ROCHE-model fit to all broadening functions. The panels give the orbital phase and the heliocentric Julian date (with 2 400 000 subtracted). |
Open with DEXTER |
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Fig. 6
continued. |
Open with DEXTER |
![]() |
Fig. 6
continued. |
Open with DEXTER |
![]() |
Fig. 6
continued. |
Open with DEXTER |
© ESO, 2011
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