EDP Sciences
Free Access
Volume 582, October 2015
Article Number A44
Number of page(s) 15
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/201526002
Published online 05 October 2015

Online material

Appendix A: AMBER interferometric results 26 December 2012

thumbnail Fig. A.1

AMBER observation of HD 98922 at spectral resolution of R = 12 000 (26 Dec. 2012). From top to bottom: wavelength dependent flux, visibilities, wavelength-differential phases, and closure phases observed at three different projected baselines (see labels in figure). For clarity, the differential phases of the first and last baselines are shifted by +30° and 30°, respectively.

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Appendix B: Modelling results for disc-wind model P5 and symmetric disc model

thumbnail Fig. B.1

Comparison of our interferometric observations with the interferometric observables derived from our best disc-wind model P5 plus the symmetric disc model described in Sect. 6.2. From top to bottom, observed Brγ line profile (grey) and model line profile (pink), observed visibilities (grey dots with error bars) and model visibilities (coloured lines), observed and model wavelength-differential phases, and observed and model closure phase.

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© ESO, 2015

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