We note however
parenthetically that the observations of polarization at high densities
(
cm-3) where radiation fields can hardly be of
importance represent a serious challenge to grain alignment theorists.
In fact, recent work shows that radiative torques due to starlight are
required to drive grains to the suprathermal rotation rates necessary
to minimize the disaligning effect of random collisions (Draine &
Weingartner 1996, 1997).
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