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Fig. 2

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Comparison between photometric/spectroscopic observations and DUSTY best-fit models for AGB stars. The left panel is for a selected O-rich star and the right panel for a C-rich star. The solid lines are ISO SWS spectra in the range between 2.5 μm and 45 μm. The diamonds represent 2MASS J, H, and Ks-band fluxes and ISO synthetic photometry for W1, W2, W3, and W4. The dotted lines are the best-fit models described in the text. The molecular features discussed in the text are marked.

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