  The recent detection of resolved radio emission from AG Dra by MERLIN
reported by Ogley et al. is discussed in the context of the wind environment
and the physical parameters and geometry of this symbiotic binary system. In
particular, it is shown that the two radio components are closely aligned with
the binary axis, and their separation suggests their origin in jets ejected
from AG Dra during the recent 1995--98 series of oubtbursts.
