VLTI-AMBER velocity-resolved aperture-synthesis imaging of η Carinae with a spectral resolution of 12 000 - Studies of the primary star wind and innermost wind-wind collision zone

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Fig. B.1

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Continuum-subtracted Brγ images (see Sect. 4 and Appendix B; the FOV of the images is 50 × 50 mas or 118 × 118 au). The continuum-normalized spectrum at the top is the average of all spectra of the data listed in Table 1. The white crosses mark the central position of the continuum wind.

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