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Variability is a key characteristic of young stars. Two major origins may be distinguished: a scaled‐up version of the magnetic activity seen on main‐sequence stars and various processes related to circumstellar disks, accretion, and outflows. (© 2015 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)

Variabiity of young stellar objects: Accretion, disks, outflows, and magnetic activity