Best-fit results with 3σ uncertainties of the power-law models from Ertel et al. (2014).
|One-component model||Two-component model|
|Inner disc||Outer disc|
|M d [M⊕]||1.3 × 10-2||2.1 × 10-4||1.1 × 10-2|
Notes. The dust surface number density is defined as n ∝ sγrα. r1 and r2 are the inner and outer boundaries of a disc, θ is the disc inclination from face-on, and Md the dust mass for particles with radii s< 1 mm. Values marked with
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