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- W3105494938 abstract "Chromospheric activity has been thought to decay smoothly with time and, hence, to be a viable age indicator. Measurements in solar-type stars in open clusters seem to point to a different conclusion: chromospheric activity undergoes a fast transition from Hyades level to that of the Sun after about 1 Gyr of main-sequence lifetime and any decaying trend before or after this transition must be much less significant than the short-term variations." @default.
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- W3105494938 date "2010-02-19" @default.
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- W3105494938 title "The discontinuous nature of chromospheric-activity evolution" @default.
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- W3105494938 doi "https://doi.org/10.1007/s10509-010-0310-5" @default.
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