  We present sensitive, high angular resolution ($0\rlap.{''}05$) VLA continuum
observations made at 7 mm of the core of the HH 111/121 quadrupolar outflow. We
estimate that at this wavelength the continuum emission is dominated by dust,
although a significant free-free contribution ($\sim$30%) is still present. The
observed structure is formed by two overlapping, elongated sources
approximately perpendicular to each other as viewed from Earth. We interpret
this structure as either tracing two circumstellar disks that exist around each
of the protostars of the close binary source at the core of this quadrupolar
outflow or a disk and a jet perpendicular to it. Both interpretations have
advantages and disadvantages, and future high angular resolution spectroscopic
millimeter observations are required to favor one of them in a more conclusive
way.
