Constraining the turbulence and the dust disk in IM Lup: Onset of planetesimal formation

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Table 4

IM Lup best fit parameters of Eqs. (20)–(22).

Parameter	Value
^q
^p
a₀
ε₀
γ
α_turb

Notes. The fit values and the uncertainties are given by the 16th, 50th, and 84th percentiles of the samples in the marginalized distributions.

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