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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 23.
Same as Figure 15, but for simulations G101Dn6In4n3 and G101Dn6In4n4m5.
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© 2026. The Author(s). Published by the American Astronomical Society.
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