The impact of disk-locking on convective turnover times of low-mass pre-main sequence and main sequence stars

Abstract

Aims. The impact of disk-locking on the stellar properties related to magnetic activity from the theoretical point of view is investigated. Methods. We use the ATO

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EDP Sciences OAI-PMH repository (1.2.0)

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Last time updated on 12/12/2024

This paper was published in EDP Sciences OAI-PMH repository (1.2.0).

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