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The ISO-SWS Spectrum of IRAS 03313+6058-an Extreme C-rich star
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作者 Jiang B.W. (Beijing Astronomical Observatory, The Chinese Academy of Sciences, Beijing 100012, China) 《天文研究与技术》 CSCD 1999年第S1期240-244,共5页
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.... 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. 展开更多
关键词 IRAS Extreme C-rich star The ISO-SWS Spectrum of IRAS 03313+6058-an ISO SWS
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