How drifting and evaporating pebbles shape giant planets - I. Heavy element content and atmospheric C/O

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This article has an erratum: [https://doi.org/10.1051/0004-6361/202141096e]

Table J.1.

Fit results for Fig. 13.

simulation	ϵ₀ = 1 × 10⁻²	ϵ₀ = 1.5 × 10⁻²	ϵ₀ = 2 × 10⁻²	ϵ₀ = 2.5 × 10⁻²
plain	6.4 ± 0.3	7.5 ± 0.3	9.7 ± 0.3	11.5 ± 0.4
evap	28.6 ± 1.6	47.3 ± 3.6	65.1 ± 7.7	82.1 ± 11.4

(a) Fit parameter γ_a

simulation	ϵ₀ = 1 × 10⁻²	ϵ₀ = 1.5 × 10⁻²	ϵ₀ = 2 × 10⁻²	ϵ₀ = 2.5 × 10⁻²

plain	0.65 ± 0.02	0.70 ± 0.02	0.69 ± 0.01	0.70 ± 0.01
evap	0.53 ± 0.02	0.49 ± 0.03	0.52 ± 0.05	0.54 ± 0.06

(b) Fit parameter γ_b

Notes: The total heavy element content is related to the final mass by the power law M_Z = γ_a ⋅ M^γ_b.

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