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Fig. 2


Comparison between the mid-IR synthetic spectra and the MIDI calibrated spectra and between the near-IR photometry and K-band synthetic spectrum for S Ser. The spectra were not fitted but used as constraints to model the visibilities.The synthetic spectra for the N band are based on the three-layer model, one per range of wavelengths: 7.809.30 μm, 9.3711.50 μm, and 11.5513.26 μm. The light gray spectrum model for S Ser has been obtained fitting the visibilities with a single envelope.

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