A new high-velocity molecular outflow of IRAS 19282+1814

We made mapping observation in the 12CO J=1-0 line which revealed the existence of a blue-shifted monopolar high-velocity molecular outflow near IRAS19292+1814. The parameters of this outflow are calculated. As indicated by the IRAS color indices, the associated infrared source IRAS19292+1814 may be a massive young stellar object (YSO) deeply embedded in the surrounding gas and dust. There is no other source nearby, so IRAS19292+1814 probably is the driving source of the outflow.