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Fig. 1.


Prediction of the model described by Eq. (9) for different values of p (various red lines) and for a mass-radius slope γ = 1.4 (upper panel) and γ = 2.38 (lower panel), using results obtained in the samples of Urquhart et al. (2018) and Traficante et al. (2018a), respectively. The models have been normalized to all have = 1 at M0 ≤ 300 M. The azure-dashed lines are the -mass relations found in Urquhart et al. (2018, upper panel) and Traficante et al. (2018a, lower panel) respectively, normalized to have = 1 at M0 = 150 M for ease of visualization.

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