The first detection of 3-5% circular polarization in radio continuum toward a massive protostar yields a model-dependent magnetic field estimate of 20-35 G near the star.
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First detection of Circular Polarization in radio continuum towards a Massive Protostar
The first detection of 3-5% circular polarization in radio continuum toward a massive protostar yields a model-dependent magnetic field estimate of 20-35 G near the star.