Magnetic Fields in Massive Star-forming Regions (MagMaR). VII. On the dynamical importance of B-fields in massive protocluster W33 A
Published in Astronomy & Astrophysics, accepted, 2026
ALMA polarization observations of W33 A show how magnetic fields can stabilize filaments, regulate accretion, and delay core collapse within a single massive protocluster.
Recommended citation: Xu, F., Zhang, Q., Sanhueza, P., Wang, K., et al. (2026). "Magnetic Fields in Massive Star-forming Regions (MagMaR). VII. On the dynamical importance of B-fields in massive protocluster W33 A." Astronomy & Astrophysics, accepted.
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