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- W2187780666 abstract "Based on Kurucz (1992) grid of models the NLTE calculations of nitrogen abundance in Peg atmosphere re- vealed a slight deficiency of this element comparably to so- lar value ((N=H) 0:3). Together with the recent result on carbon abundance in this star atmosphere ((C=H )= 0:25; Korotin et al., 1998), the present determination shows that tur- bulent diffusion in massive main sequence stars (discussed by Maeder, 1987) and connected with it the appearance of the CN- processed material at the stellar surface can hardly be operating in Peg. The list of Nii lines that can be used for LTE calculation of nitrogen abundance in hot stars is also presented." @default.
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- W2187780666 date "1999-01-01" @default.
- W2187780666 modified "2023-09-27" @default.
- W2187780666 title "I. NLTE calculations for Pegasi" @default.
- W2187780666 hasPublicationYear "1999" @default.
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