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Silicon carbide absorption features: dust formation in the outflows of extreme carbon stars
ASTROPHYSICAL JOURNAL, no. 2 (2009): 1202-1221
摘要
Infrared carbon stars without visible counterparts are generally known as extreme carbon stars. We have selected a subset of these stars with absorption features in the 10-13 mu m range, which has been tentatively attributed to silicon carbide (SiC). We add three new objects meeting these criterion to the seven previously known, bringing ...更多
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