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We investigate the alignment between outflow axes in nine of the youngestbinary/multiple systems in the Perseus Molecular Cloud. These systems havetypical member spacing larger than 1000 AU. For outflow identification, we use12CO(2-1) and 12CO(3-2) data from a large survey with the Sub- millimeterArray: Mass Assembly of Stellar Systems and their Evolution with the SMA(MASSES). The distribution of outflow orientations in the binary pairs isconsistent with random or preferentially anti-aligned distributions,demonstrating that these outflows are misaligned. This result suggests thatthese systems are possibly formed in environments where the distribution ofangular momentum is complex and disordered, and these systems do not come fromthe same co-rotating structures or from an initial cloud with aligned vectorsof angular momentum.

Misalignment of Outflow Axes in the Proto-Multiple Systems in Perseus