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Table 3

Continuum and CO radial extension for each source.

R% Rdust [au] [au] [au] RgasRdust
(Rgas)
CIDA 1 68 73.7 ± 15.0 47.4 ± 6.8 3.0 ± 0.6
90 108.1 ± 15.0 68.5 ± 6.8 3.7 ± 0.5
MHO 6 68 130.7 ± 7.0 78.5 ± 7.1 3.8 ± 0.2
90 191.9 ± 7.0 113.0 ± 7.1 4.1 ± 0.2
J0433 68 114.6 ± 11.9 92.2 ± 11.7 3.1 ± 0.3
90 174.0 ± 11.9 125.5 ± 11.7 3.8 ± 0.3
CIDA 7 68 55.1 ± 10.8 19.6 ± 10.9 6.0 ± 1.2
90 78.9 ± 10.8 6.0 ± 0.8
J0420 68 43.1 ± 9.9 23.3 ± 9.8 2.9 ± 0.7
90 57.7 ± 9.9 32.2 ± 9.8 2.7 ± 0.5
J0415 68 26.4 ± 12.1 2.4 ± 1.2
90 34.8 ± 12.1 2.3 ± 0.9

Notes. Uncertainties for continuum comes from the walkers distribution in each MCMC. Gas radii uncertainties were calculated from the synthesized beam radius of each image.

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