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- W2055775360 abstract "Chromospheric emission in the Ca II H and K lines has often been used as an age diagnostic for solar mass stars. For 20 such stars with ages less than a few hundred megayears, we compare Ca II ages derived by Wright et al. with ages we derive based on a combination of lithium abundance, X-ray activity, and Galactic space motion. Typically, the Ca II ages are noticeably older than the lithium/X-ray ages, suggesting that a recalibration of the Ca II ages may be necessary." @default.
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- W2055775360 date "2004-09-21" @default.
- W2055775360 modified "2023-10-03" @default.
- W2055775360 title "On Ca <scp>ii</scp> Emission as an Indicator of the Age of Young Stars" @default.
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- W2055775360 doi "https://doi.org/10.1086/425683" @default.
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