Grain opacity and the bulk composition of extrasolar planets - I. Results from scaling the ISM opacity

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Fig. A.5

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Mass of a core M_Z,0,crit that undergoes gas runaway accretion after being embedded in the nebula without planetesimal accretion during a time t. The solid black line uses the parameters for τ_g from Ikoma et al. (2000) while the dashed blue line is for the updated parameters of Ikoma & Genda (2006).

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