摘要
The ISO-SWS spectrum of IRAS03313+6058 is presented. The spectral energy distribution in the full coverage of ISO-SWS between 2 3 and 45μm 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 14μm, wide emission band around 30μm and emission bands around 41 ad 43 5μm.
The ISO-SWS spectrum of IRAS03313+6058 is presented. The spectral energy distribution in the full coverage of ISO-SWS between 2 3 and 45μm 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 14μm, wide emission band around 30μm and emission bands around 41 ad 43 5μm.
出处
《天文研究与技术》
CSCD
1999年第S1期240-244,共5页
Astronomical Research & Technology
