Abstract
We report a discovery of multiple outflows in IRAS 06056+2131. The highangular resolution image (~15′′) of CO (1–0) emission revealsthat the structure of outflow is very complicated. The outflow appearsto be everywhere. Its configuration only show a bipolar outflow atobservation of both low resolution and low signal-to-noise ratio, whiletwo bipolar outflows can be detected when observed by both highresolution and high signal-to-noise ratio mapping. This result issignificant in the understanding of the physical processes that occur atearly phase of massive stars.
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