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• W2057181013 abstract "Context.A recent analysis of visual Fe ii emission lines of 17 classic Be stars using the self-absorption curve (SAC) method revealed that these lines are optically thick and that they form in circumstellar disc (CD) regions within two stellar radii from the central star on average." @default.
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• W2057181013 date "2007-05-10" @default.
• W2057181013 modified "2023-10-15" @default.
• W2057181013 title "Be star disc characteristics near the central object" @default.
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• W2057181013 doi "https://doi.org/10.1051/0004-6361:20066615" @default.
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