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method:computer-simulation-of-spiral-galaxy-formation

Computer Simulation of Spiral Galaxy Formation

Computational modeling of the emergence of two-armed spiral structure from a perturbed rotating galactic disk, showing smooth structure-preserving transitions

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cosine ≥ 0.65 · no typed edge

Entities in the same semantic neighborhood but without a typed relation to this one — candidates for new edges or unrecognized duplicates.