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Fig. 19


Comparison of the type of planets formed using the nominal case grain opacity (which is the full interstellar one) and a reduced one (by a factor fopa =0.01) for the model computing the internal structure. Top panel: starting time of t = 1.5 Myr and the bottom panel for t = 2 Myr. The green line represents the results of Mayor et al. (2011) for planets beyond 0.1 AU for comparison.

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