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Showing 1 to 1 of 1 for “"Subarcsecond"”.
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Observations of disks around the youngest protostars: Characterizing frequency, dust properties, and magnetic fields at the earliest times
… by the magnetic fields of the system? We examine subarcsecond (∼0.35′′) resolved CARMA polarization observations of the 1.3 mm dust polarization from the disk around the Class 0 protostar L1527 to understand the inferred magnetic field morphology of the system on 50 AU size scales. L1527 is the …