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• W3100157689 abstract "Context. Despite their carbon-rich photospheres, silicate carbon stars show 10 μm silicate emission. They are considered to have circumbinary or circum-companion disks, which serve as a reservoir of oxygen-rich material shed by mass loss in the past." @default.
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• W3100157689 date "2008-08-25" @default.
• W3100157689 modified "2023-10-16" @default.
• W3100157689 title "Asymmetric silicate dust distribution toward the silicate carbon star BM Geminorum" @default.
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• W3100157689 doi "https://doi.org/10.1051/0004-6361:200810229" @default.
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