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Chemical composition and origin of nebulae around Luminous Blue Variables
ASTROPHYSICAL JOURNAL, no. 2 (2001): 764-780
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We use the analysis of the heavy element abundances (C, N, O, S) in circumstellar nebulae around luminous blue variables to infer the evolutionary phase in which the material has been ejected. We concentrate on four aspects. (1) We discuss the different effects that may have changed the gas composition of the nebula since it was ejected :...更多
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