Formation of planetary systems by pebble accretion and migration - Hot super-Earth systems from breaking compact resonant chains

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Fig. 9

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Same as Fig. 8, except that we now use rocky pebbles of Rocky_peb = 1 cm. This leads to enhanced growth of the inner embryos in contrast to Fig. 8. The efficiency of pebble accretion is about 5.6, 4.8, 4.1, and 3.4% for S_peb = 1, 2.5, 5, and 10, respectively.

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