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

Astronomische Nachrichten (2015) 336(5) 493-498
DOI: 10.1002/asna.201512185
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Abstract

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).

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Stelzer, B. (2015). Variabiity of young stellar objects: Accretion, disks, outflows, and magnetic activity. Astronomische Nachrichten, 336(5), 493–498. https://doi.org/10.1002/asna.201512185

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