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- W400133089 abstract "We are motivated to study the Ne/He abundance ratio at the surfaces of Wolf-Rayet stars by evolutionary models, which have predicted enhancements by more than an order of magnitude over cosmic levels during the WC stage ( e.g. , Maeder 1991). This should occur early in the WC phase, as core-hydrogen is exhausted and the CNO bi-cycle gives way to the following chain of reactions for the Galactic stars: The latest evolutionary models, which include the effects of interior mixing due to stellar rotation, indicate that the enhancement may be somewhat more gradual, but that the Ne/He ratio is essentially unchanged in its peak value, coinciding with complete H-depletion ( e.g. , Meynet, these Proceedings)." @default.
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- W400133089 date "1999-01-01" @default.
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- W400133089 title "Neon abundances in three Wolf-Rayet stars observed with the ISO Short Wavelength Spectrometer" @default.
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- W400133089 doi "https://doi.org/10.1017/s0074180900205032" @default.
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