Magnetic field directions inferred from dust polarization show a bimodal alignment (parallel or perpendicular) with the elongation of massive protostellar cores on sub-parsec scales.
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The SOMA-POL Survey. I. Polarization and magnetic field properties of massive protostars
Magnetic field directions inferred from dust polarization show a bimodal alignment (parallel or perpendicular) with the elongation of massive protostellar cores on sub-parsec scales.