Gas dynamics around a Jupiter-mass planet - II. Chemical evolution of circumplanetary material

Open Access

Table 1

Simulation parameters from Paper 1.

Model name	$Σ_{0} / M_{⊙} r_{p}^{- 2}$ ${\Sigma _0}/{M_ \odot }r_p^{ - 2}$	$v / r_{p}^{2} Ω_{p}$ $v/r_p^2{\Omega _p}$
Nominal	6.67 × 10⁻⁴	10⁻⁵
LowMass	6.67 × 10⁻⁵	10⁻⁵
LowMassLowVis	6.67 × 10⁻⁵	10⁻⁶

Notes. Σ₀ is the initial gas density surrounding the embedded planet and v is the viscosity of the gas. r_p and Ω_p are the orbital radius of the planet and the orbital frequency at that radius. M_⊙ is the solar mass. The model that we primarily focus on is in bold, although we compute one streamline in the Nominal model.

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