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• W3100827038 abstract "Context. It is well known that stars with giant planets are, on average, more metal-rich than stars without giant planets, whereas stars with detected low-mass planets do not require to be metal-rich." @default.
• W3100827038 created "2020-11-23" @default.
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• W3100827038 date "2014-06-01" @default.
• W3100827038 modified "2023-10-16" @default.
• W3100827038 title "Chemical abundances of stars with brown-dwarf companions" @default.
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• W3100827038 doi "https://doi.org/10.1051/0004-6361/201423803" @default.
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