Polarization observations reveal dominant toroidal magnetic fields of a few milligauss in a protostellar outflow, sufficient to collimate it and supporting magneto-centrifugal launching.
A., Asgari-Targhi, M
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Unveiling Dominant Toroidal Magnetic Fields in a Protostellar Outflow
Polarization observations reveal dominant toroidal magnetic fields of a few milligauss in a protostellar outflow, sufficient to collimate it and supporting magneto-centrifugal launching.