ALMA data and simulations show turbulence dominates magnetism in forming massive star cluster seeds, with condensations aligning parallel rather than perpendicular to B fields.
K.et al.The Jeans Condition: A New Constraint on Spatial Resolution in Simulations of Isothermal Self-gravitational Hydrodynamics.Astrophys
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
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.