  We examine the spatial distribution of brown dwarfs produced by the decay of
small-N stellar systems as expected from the embryo ejection scenario. We model
a cluster of several hundred stars grouped into 'cores' of a few stars/brown
dwarfs. These cores decay, preferentially ejecting their lowest-mass members.
Brown dwarfs are found to have a wider spatial distribution than stars, however
once the effects of limited survey areas and unresolved binaries are taken into
account it can be difficult to distinguish between clusters with many or no
ejections. A large difference between the distributions probably indicates that
ejections have occurred, however similar distributions sometimes arise even
with ejections. Thus the spatial distribution of brown dwarfs is not
necessarily a good discriminator between ejection and non-ejection scenarios.
