The ISO-SWS spectrum of IRAS 03313+6058 - an extreme C-rich star.

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Carbon Stars: Stellar Spectra

Scientific paper

The ISO-SWS spectrum of IRAS 03313+6058 is presented. The spectral energy distribution in the full coverage of ISO-SWS between 2.3 and 45 μm can be fit well by assuming the amorphous carbon as the major dust component. In addition, a few evident spectral features are found, including the absorption bands around 7.5 and 14 μm, wide emission band around 30 μm, and emission bands around 41 and 43.5 μm.

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