Dust in brown dwarfs and extra-solar planets - VI. Assessing seed formation across the brown dwarf and exoplanet regimes

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Fig. 13

Left: number density contours of CsCl gas phase monomers, log₁₀ n(CsCl) [cm⁻³]. Right: CsCl[s] S = 1 phase equilibrium result (thick black, solid) and nucleation rate log₁₀ J _* contour lines (black, dashed), compared to the S = 1 equilibrium limit equations (coloured, solid) found in Visscher et al. (2006, 2010), Morley et al. (2012), Wakeford et al. (2017b) for a variety of cloud condensate species.

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