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IRAS 19111+2555(=S Lyr):A Possible Silicate Carbon Star
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作者 Pei-ShengChen Xun-HaoWang 《Chinese Journal of Astronomy and Astrophysics》 CSCD 北大核心 2001年第4期344-348,共5页
The properties and classification of IRAS 19111+2555 have so far not been well determined. We collect all the available information and data of this star, and take the data obtained by IRAS LRS and ISO SWS to discuss ... The properties and classification of IRAS 19111+2555 have so far not been well determined. We collect all the available information and data of this star, and take the data obtained by IRAS LRS and ISO SWS to discuss its properties and classification. The star is found to have a 3.1μm feature in absorption and a 10μm feature in emission, so it is possibly a new silicate carbon star. 展开更多
关键词 stars: AGB and post-AGB - stars: carbon - infrared: stars
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