In IC 348, 90 of 127 young stars show significant Hα equivalent-width variability, and the variable stars are systematically more massive and more active than non-variables.
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Variability of Ha emission in young stellar objects in the cluster IC 348
In IC 348, 90 of 127 young stars show significant Hα equivalent-width variability, and the variable stars are systematically more massive and more active than non-variables.