ALMA data and simulations show turbulence dominates magnetism in forming massive star cluster seeds, with condensations aligning parallel rather than perpendicular to B fields.
T.et al.Self-similarity of the magnetic field at different scales: The case of G31.41+0.31.Astron
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The dominance of turbulence over magnetism in the formation of massive star cluster seeds
ALMA data and simulations show turbulence dominates magnetism in forming massive star cluster seeds, with condensations aligning parallel rather than perpendicular to B fields.