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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Maser emissions act as cosmic rulers for astrometric measurements of astronomical sources from protostellar scales to galactic distances, with SKA-Mid enabling expanded multi-species observations.
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.
citing papers explorer
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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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Cosmic Rulers: Masers as Tools for Probing Structure in the Galaxy and Beyond, from AU to kpc
Maser emissions act as cosmic rulers for astrometric measurements of astronomical sources from protostellar scales to galactic distances, with SKA-Mid enabling expanded multi-species observations.
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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.