Issue |
A&A
Volume 566, June 2014
|
|
---|---|---|
Article Number | A125 | |
Number of page(s) | 18 | |
Section | Stellar atmospheres | |
DOI | https://doi.org/10.1051/0004-6361/201322894 | |
Published online | 23 June 2014 |
Online material
Appendix A: Observation logs
Observation log of AMBER.
Appendix B: 2006−2007 campaign
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Fig. B.1
2006−2007 Hα time series of Rigel obtained with FEROS. |
Open with DEXTER |
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Fig. B.2
2006−2007 Brγ time series of Rigel obtained with AMBER. |
Open with DEXTER |
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Fig. B.3
Differential visibilities of Rigel obtained in 2006−2007 and put to the scale corresponding to an angular diameter of 2.75 mas. The visibilities are compared with the ones computed from CMFGEN models tuning the mass-loss rate only. |
Open with DEXTER |
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Fig. B.4
Differential phases and photocentre shift of Rigel obtained in 2006−2007. |
Open with DEXTER |
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Fig. C.1
2009−2010 Hα time series of Rigel obtained with BESO. |
Open with DEXTER |
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Fig. C.2
2009−2010 Brγ time series of Rigel obtained with AMBER. |
Open with DEXTER |
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Fig. C.3
Differential visibilities of Rigel obtained obtained in 2009−2010 and put to the scale corresponding to an angular diameter of 2.75 mas. The visibilities are compared with the ones computed from CMFGEN models with varying mass-loss rate. |
Open with DEXTER |
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Fig. C.4
Differential visibilities of Rigel obtained in 2009−2010 (continued). |
Open with DEXTER |
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Fig. C.5
Differential phases and photocentre shift of Rigel obtained in 2009−2010. |
Open with DEXTER |
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Fig. C.6
Differential phases and photocentre shift of Rigel obtained in 2009−2010 (continued). At MJD = 55 267.099 (upper row), the baselines were aligned preventing the computation of a 2D photocentre. |
Open with DEXTER |
© ESO, 2014
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