We present archival high angular resolution ( \sim 2 ^ { \prime \prime } ) ^ { 12 } CO ( 3-2 ) line and continuum submillimeter observations of the young stellar object HL Tau made with the Submillimeter Array ( SMA ) .
The ^ { 12 } CO ( 3-2 ) line observations reveal the presence of a compact and wide opening angle bipolar outflow with a northeast and southwest orientation ( P.A .
= 50 ^ { \circ } ) , and that is associated with the optical and infrared jet emanating from HL Tau with a similar orientation .
On the other hand , the 850 \micron continuum emission observations exhibit a strong and compact source in the position of HL Tau that has a spatial size of \sim 200 \times 70 AU with a P.A . = 145 ^ { \circ } , and a dust mass of around 0.1 M _ { \odot } .
These physical parameters are in agreement with values obtained recently from millimeter observations .
This submillimeter source is therefore related with the disk surrounding HL Tau .