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- W2054795707 abstract "A revised and updated grid of cool helium-rich model atmospheres which includes the effect of varying hydrogen abundance is used to analyze the temperature and abundance of the DZ white dwarf CBS 127. Comparisons of the star to several other DZ white dwarfs with similar T(e)s show that CBS 137 is the hottest DZ star and lies near the boundary temperature above which it has been proposed that hydrogen accretion may be prevented. Based on the results, a specifically defined single lower boundary temperature for screening is rejected, and it is demonstrated that the propeller must operate over a very broad range of T(eff), down to T(eff) as low as 5800 K, with highly variable efficiency." @default.
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- W2054795707 date "1990-10-01" @default.
- W2054795707 modified "2023-10-14" @default.
- W2054795707 title "Abundances in the hot DZ star CBS 127 - How efficient is hydrogen screening?" @default.
- W2054795707 doi "https://doi.org/10.1086/169306" @default.
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