Abstract
We present sensitive, high angular resolution (0''.3) Very Large Array observations made at 3.6 cm of the bright infrared source AFGL 4029. We find that the radio source G 138.295+1.555, associated with AFGL 4029-IRS1, is actually a subarcsecod binary. There is also fainter emission extending in the east-west direction and emanating from G 138.295+1.555(S), the southern component of the binary. We then identify G 138.295+1.555(S) as the exciting source of the optical and molecular outflow observed in this region.
