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- W3100933089 abstract "Knowledge of the metallicities of M dwarfs rests predominantly on the photometric calibration of Bonfils and collaborators, which predicts that M dwarfs in the solar neighborhood, including those with known planets, are systematically metal poor compared to their higher-mass counterparts. We test this prediction using a volume-limited sample of low-mass stars, together with a subset of M dwarfs with high-metallicity, F, G, and K wide binary companions. We find that the Bonfils et al. photometric calibration systematically underestimates the metallicities of our high-metallicity M dwarfs by an average of 0.32 dex. We derive a new photometric metallicity calibration and show that M dwarfs with planets appear to be systematically metal rich, a result that is consistent with the metallicity distribution of FGK dwarfs with planets." @default.
- W3100933089 created "2020-11-23" @default.
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- W3100933089 date "2009-06-17" @default.
- W3100933089 modified "2023-10-17" @default.
- W3100933089 title "ON THE METAL RICHNESS OF M DWARFS WITH PLANETS" @default.
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- W3100933089 doi "https://doi.org/10.1088/0004-637x/699/2/933" @default.
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