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Fig. 5


Relative response curves of the AKARI 9 μm band and 18 μm band. The ISO/SWS spectra of typical Galactic C-rich and O-rich stars are overlaid as references (Sloan et al. 2003). An example of the C-rich star, IRC +40540, displays carbonaceous features around 11 and 30 μm, that are not covered by the AKARI bands. A typical O-rich star, oCet, shows silicate features around 10 and 18 μm, which are efficiently covered by the AKARI bands.

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