Polarization observations of 6.7 GHz methanol masers show linear and circular components with Zeeman splitting that varies over time, interpreted as evidence for changing magnetic fields.
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The paper presents predictions and observational plans for Zeeman effect measurements with SKA to provide statistical data on magnetic field strengths across scales in molecular clouds.
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Polarization Observations of a Sample of 6.7 GHz Methanol Masers
Polarization observations of 6.7 GHz methanol masers show linear and circular components with Zeeman splitting that varies over time, interpreted as evidence for changing magnetic fields.
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Measuring Magnetic Field Strengths in Galactic Star-forming Regions via the Zeeman Effect with the SKA
The paper presents predictions and observational plans for Zeeman effect measurements with SKA to provide statistical data on magnetic field strengths across scales in molecular clouds.