EDP Sciences
Free Access
Issue
A&A
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.

Open with DEXTER

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.

Open with DEXTER


© ESO, 2015

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.