  The Bok globule CB230 (L1177) contains an active, low-mass star-forming core
which is associated with a double NIR reflection nebula, a collimated bipolar
molecular outflow, and strong mm continuum emission. The morphology of the NIR
nebula suggests the presence of a deeply embedded, wide binary protostellar
system. High-angular resolution observations now reveal the presence of two
sub-cores, two distinct outflow centers, and an embedded accretion disk
associated with the western bipolar NIR nebula. In terms of separation and
specific angular momentum, the CB230 double protostar system probably results
from core fragmentation and can be placed at the upper end of the pre-main
sequence binary distribution.
