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Paper: Empirical Constraints on the Interiors of Low-Mass Pre-Main-Sequence Stars and Young Brown Dwarfs
Volume: 384, 14th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun
Page: 214
Authors: Stassun, K.G.
Abstract: We draw upon recent results from efforts to directly and accurately measure the fundamental physical properties of young, low-mass stars and brown dwarfs that provide insights on the interiors of these objects. Specifically, there is emerging evidence for suppressed convection in young low-mass stars and brown dwarfs, and that this suppression is connected to magnetic activity.
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