High-resolution dust polarization and C18O observations in Cepheus A show gravity driving gas accretion while magnetic tension regulates turbulence, producing ordered flows at 2.1e-4 solar masses per year with coherent B-field alignment across scales.
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Evidence for the gravity-driven and magnetically-regularized gas flows feeding the massive protostellar cluster in Cepheus A
High-resolution dust polarization and C18O observations in Cepheus A show gravity driving gas accretion while magnetic tension regulates turbulence, producing ordered flows at 2.1e-4 solar masses per year with coherent B-field alignment across scales.