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• W2161482777 abstract "Context. The Be stars are massive dwarf or subgiant stars that present temporary emission lines in their spectrum, and particularly in the Hα line. The mechanism triggering these Be episodes is currently unknown, but binarity could play an important role." @default.
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• W2161482777 date "2008-04-22" @default.
• W2161482777 modified "2023-10-13" @default.
• W2161482777 title "The close-in companion of the fast rotating Be star Achernar" @default.
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• W2161482777 doi "https://doi.org/10.1051/0004-6361:200809765" @default.
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