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Interactions between the Planetary Magnetic Field and the Surrounding Gas Flows in the Final Stage of the Giant Planet Formation. I. Two Distinct Evolutionary Scenarios
Pengfei Tang et al 2026 The Astrophysical Journal 1005 .
Caption: Figure 24.
Same as Figure 15, but for simulations G105Dn5In3 and G105Dn5In3n4m5.
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© 2026. The Author(s). Published by the American Astronomical Society.
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