Fig. 3.
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Gas density distribution at successive moments in main-sequence star collisions with M1 = 1 M⊙, M2 = 0.9 M⊙, Vrel = 5000 km s−1, but different impact parameters. These AREPO simulations of stellar collisions are characterized by b = 0.1, 0.25, and 0.5 (from top to bottom) and shown here at t = 0.0, 0.01, 0.05, and 0.5 d (from left to right).
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