Metallicity effect and planet mass function in pebble-based planet formation models

N. Brügger; Y. Alibert; S. Ataiee; W. Benz

doi:10.1051/0004-6361/201833347

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Volume 619 (November 2018)

A&A, 619 (2018) A174

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Fig. 2

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As in Fig. 1 but using Eq. (15) to compute the flux of pebbles. The match with the results of B15b is much better (the thin lines are barely visible but there is one such line below each of the thick lines).

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