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- W2006599439 abstract "A differential curve of growth analysis of three K-giant stars (HD 2490, HD 130227 and HD 130694) assigned membership in Eggen's σ Pup moving group is carried out relative to α B00. This group is believed to represent a sample of very old disk population stars. The abundances of five elements in these stars do not differ greatly from α Boo, having [Fe/H] ≈ – 0·5. This result agrees with those of Williams and Boyle & McClure using narrow and intermediate band photometry respectively." @default.
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- W2006599439 date "1976-10-01" @default.
- W2006599439 modified "2023-10-08" @default.
- W2006599439 title "On Element Abundances in Stars Belonging to the Puppis Group" @default.
- W2006599439 doi "https://doi.org/10.1093/mnras/177.1.3" @default.
- W2006599439 hasPublicationYear "1976" @default.
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