ALMA data and simulations show turbulence dominates magnetism in forming massive star cluster seeds, with condensations aligning parallel rather than perpendicular to B fields.
M.et al.Resolving the Polarized Dust Emission of the Disk around the Massive Star Powering the HH 80-81 Radio Jet.Astrophys
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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.