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Where Do Hot Jupiters Come from? Revisiting Tidal Disruption and Ejection in High-eccentricity Migration

  • Authors: Qianli Fan, 千里 范, Shang-Fei Liu, 尚飞 刘

Qianli Fan et al 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure 6.

Density (left) and cumulative mass (right) profiles for planetary models with a 20M⊕ core, under different mass-loss scenarios: no mass loss, 50% mass loss, and 80% mass loss. The blue solid, orange dashed, and green dotted lines correspond to total masses of 1.0MJ, 0.5MJ, and 0.2MJ, respectively.

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