Brown dwarfs forming in discs: Where to look for them?

A large fraction of the observed brown dwarfs may form by gravitational fragmentation of unstable discs. This model reproduces the brown dwarf desert, and provides an explanation for the existence of planetary-mass objects and for the binary properties of low-mass objects. We have performed an ensem...

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Bibliographic Details
Main Authors: Stamatellos D., Whitworth A.
Format: Article
Language:English
Published: EDP Sciences 2011-07-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20111605001