  In the traditional picture of black holes Hawking radiation is created by
pair creation from the vacuum at the horizon. In the fuzzball proposal,
individual microstates do not have a horizon with the `vacuum' state in its
vicinity. For a special family of non-extremal microstates it was recently
found that emission occurs due to pair creation in an ergoregion, rather than
at a horizon. In this paper we extend this result to a slightly larger class of
microstates, again finding exact agreement between the emission in the gravity
picture and the CFT dual. We write down an expression for emission from
geometries with ergoregions, in terms of the leading falloff behavior of the
wavefunctions in the fuzzball region. Finally, we describe another family of
nonextremal microstates and find their ergoregion.
