SMA, VLA and VLBA observations in a 105 L⊙ high mass star formation region IRAS 18360-0537

We have observed a young stellar object, IRAS 18360-0537, with a far-infrared luminosity of 1.2 × 10⁵ L_⊙. It is perhaps the most promising candidate of a high-mass protostar associated with a Keplerian disk and a jet/outflow system in the regime of L > 10⁵L_⊙. We are conducting the SMA, VLA, and VLBA studies to provide a comprehensive understanding of this interesting high mass star formation scenario.