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- W2024454474 abstract "The abundances of eight elements (C through Fe) were determined in the primary star of the short-period Algol-type binary RZ Cas relative to the A3 V spectroscopic standard star |$alpha$| PsA. Definite under-abundances (by |$-0.45 ,mathrm{dex}$| or more) of Mg, Si, Ti, Cr, and Fe were established. On the other hand, light elements C and O show solar abundances, and Ca is slightly under-abundant (|$sim-0.3 ,mathrm{dex}$|). This abundance pattern demonstrates that RZ Cas shows a characteristic of mild |$lambda$| Boo-type stars. This finding raises a question on the physical relations between the metallicity (abundance anomaly), the pulsational characteristics, and the mass accretion processes." @default.
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- W2024454474 date "2006-06-25" @default.
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- W2024454474 title "Discovery of a λ Bootis Like Abundance Pattern in the Pulsating Algol-Type System RZ Cassiopeiae" @default.
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- W2024454474 doi "https://doi.org/10.1093/pasj/58.3.617" @default.
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