The evolution of the Md–M⋆ and Ṁ–M⋆ correlations traces protoplanetary disc dispersal

Open Access

Table A.1

Values of the parameters used throughout the paper, unless explicitly stated otherwise.

General simulation parameters
λ_m,0	2.1
λ_acc,0	1.5
$σ_{M_{d}}$ $\[\sigma_{\mathrm{M}_{\mathrm{d}}}\]$	0.65 dex
$σ_{R_{d}}$ $\[\sigma_{\mathrm{R}_{\mathrm{d}}}\]$	0.52 dex
M_d, R_d distribution	lognormal

Viscous model

α_SS	10⁻³

Photoevaporative model

α_SS	10⁻³
${\dot{M}}_{w}$ $\[\dot{M}_w\]$	4 × 10⁻¹⁰ M_⊙ yr⁻¹

Wind-driven model

α_SS	10⁻³
α_DW	10⁻³
λ	3
ω	0.25

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