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The magnetic field is believed to play a crucial role in the process of starformation. From the support it provides during the initial collapse ofmolecular clouds to the creation of strong collimated jets responsible forlarge mass losses, current theories predict its importance in many differentstages during the formation of stars. Here we report on observational evidencewhich tests one aspect that can be inferred from these theories: the alignmentbetween the local magnetic field and collimated bipolar outflows in suchenvironments. There is good evidence of an alignment in the case of NGC 2071.Comment: 11 pages, 4 figure

The Alignment of the Magnetic Field and Collimated Outflows in Star‐forming Regions: The Case of NGC 2071