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- W2149577635 abstract "Context.The observed abundance peculiarities of many chemical species relative to the expected cluster metallicity in blue horizontal-branch (BHB) stars presumably appear as a result of atomic diffusion in the photosphere. The slow rotation (typically < 10 km s-1) of BHB stars with effective temperatures Teff > 11 500 K supports this idea since the diffusion mechanism is only effective in a stable stellar atmosphere." @default.
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- W2149577635 date "2007-11-06" @default.
- W2149577635 modified "2023-09-23" @default.
- W2149577635 title "Search for vertical stratification of metals in atmospheres of blue horizontal-branch stars" @default.
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- W2149577635 doi "https://doi.org/10.1051/0004-6361:20078488" @default.
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