Discovery of Multiple outflows in IRAS 06056+2131

We report a discovery of multiple outflows in IRAS 06056+2131. The high angular resolution image (～15'') of CO (1--0) emission reveals that the structure of outflow is very complicated. The outflow appears to be everywhere. Its configuration only show a bipolar outflow at observation of both low resolution and low signal-to-noise ratio, while two bipolar outflows can be detected when observed by both high resolution and high signal-to-noise ratio mapping. This result is significant in the understanding of the physical processes that occur at early phase of massive stars.