Empirical Constraints on the Interiors of Low-Mass Pre-Main-Sequence Stars and Young Brown Dwrafs

Details Empirical Constraints on the Interiors of Low-Mass Pre-Main-Sequence Stars and Young Brown Dwrafs Empirical Constraints on the Interiors of Low-Mass Pre-Main-Sequence Stars and Young Brown Dwrafs

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..384..214s&link_type=abstract

14th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun ASP Conference Series, Vol. 384, proceedings of the conferen

Physics

1

Scientific paper

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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