  We present 12CO (J=2-1) sensitive molecular line and 1.3 mm continuum
observations made with the Submillimeter Array (SMA) of the bipolar outflow
associated with the young star located in the Bok globule known as CB 26. The
SMA observations were carried out in its extended configuration allowing us to
study the kinematics and structure of the outflow with about 1 arcsec or 140 au
resolution. We find that the dusty and edge-on circumstellar disk related with
the outflow has an projected spatial (deconvolved) size of 196 au x 42 au with
a total (gas and dust) mass of 0.031 Msun. We estimated a dynamical mass for
the central object of 0.66 Msun, and the mass of the molecular outflow of
5x10-5 Msun. The observations confirm that the outflow rotation has a similar
orientation to that of the edge-on disk. For the outflow, we find that the
following quantities: the rotation velocity, the specific angular momentum, and
the launching radius, decrease with the height above mid-plane, as observed in
other molecular rotating outflows. The radius, and expansion velocity also
increase with the height above the disk midplane. Estimations for the outflow
linear momentum rate, the outflow angular momentum rate, and the accretion
luminosity seem to be well explained by a disk wind present in CB26.
