  The Be star sample of Steele et al. (1998) has a distribution of v sin i's
that is luminosity dependant, with giants having lower projected rotational
velocities than dwarfs. We show that this effect can be understood simply in
terms of angular momentum conservation during the evolution from dwarf to
giant. Any decretion disk or other angular momentum losing mechanism for such
objects must cause a loss of no more than 15 per-cent of the stellar angular
momentum over the Be phase lifetime.
