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Table A.1

Results of the MCMC fitting for the 12CO and 13CO emission of MHO 6. The uncertainties are measured from the 16th and 84th percentiles of each distribution. The fluxes (Fsky, Fcorr) and the radii (R68%, R90%, R95%) are calculated from the models, and they are not free parameters.

Parameter 12CO 13CO units Parameter 12CO 13CO units
δRA 6.31.5+1.0$6.3_{ - 1.5}^{ + 1.0}$ 7.83.7+3.3$7.8_{ - 3.7}^{ + 3.3}$ mas Ib 0.360.03+0.01$0.36_{ - 0.03}^{ + 0.01}$ 0.170.04+0.02$0.17_{ - 0.04}^{ + 0.02}$ mJy/px
δDec 5.21.8+1.3$5.2_{ - 1.8}^{ + 1.3}$ 1.64.8+5.1$1.6_{ - 4.8}^{ + 5.1}$ mas αb 0.010.01+0.01$0.01_{ - 0.01}^{ + 0.01}$ 0.040.4+0.23$0.04_{ - 0.4}^{ + 0.23}$
inc 59.10.5+2.8$59.1_{ - 0.5}^{ + 2.8}$ 59.61.4+1.7$59.6_{ - 1.4}^{ + 1.7}$ deg βb 2.950.06+0.38$2.95_{ - 0.06}^{ + 0.38}$ 1.920.06+0.69$1.92_{ - 0.06}^{ + 0.69}$
PA 293.50.3+0.2$293.5_{ - 0.3}^{ + 0.2}$ 293.80.9+0.5$293.8_{ - 0.9}^{ + 0.5}$ deg

M 0.1640.003+0.003$0.164_{ - 0.003}^{ + 0.003}$ 0.1710.010+0.009$0.171_{ - 0.010}^{ + 0.009}$ M δυ0 457.97.4+6.6$457.9_{ - 7.4}^{ + 6.6}$ 780.942.4+48.3$780.9_{ - 42.4}^{ + 48.3}$ m s−1
VLSR 5627.03.6+3.8$5627.0_{ - 3.6}^{ + 3.8}$ 5690.913.4+13.4$5690.9_{ - 13.4}^{ + 13.4}$ m s−1 q 0.400.02+0.02$0.40_{ - 0.02}^{ + 0.02}$ 0.150.05+0.05$0.15_{ - 0.05}^{ + 0.05}$
δυmax <1371.444.5+430.8$ < 1371.4_{ - 44.5}^{ + 430.8}$ <1466.7309.5+359.8$ < 1466.7_{ - 309.5}^{ + 359.8}$ m s−1

rɀ 49.56.9+46.8$49.5_{ - 6.9}^{ + 46.8}$ 105.14.6+138.3$105.1_{ - 4.6}^{ + 138.3}$ au Clυ0 2.614.2+14.4$2.6_{ - 14.2}^{ + 14.4}$ 6.172.6+81.8$ - 6.1_{ - 72.6}^{ + 81.8}$ m s−1
rI 152.10.1+3.5$152.1_{ - 0.1}^{ + 3.5}$ 98.12.05+10.0$98.1_{ - 2.05}^{ + 10.0}$ au Clσ 986.270.9+77.1$986.2_{ - 70.9}^{ + 77.1}$ 563.3151.4+180.9$563.3_{ - 151.4}^{ + 180.9}$ m s−1
rmax <839.5450.1+49.5$ < 839.5_{ - 450.1}^{ + 49.5}$ <578.3287.0+283.8$ < 578.3_{ - 287.0}^{ + 283.8}$ au Cla 0.470.02+0.02$0.47_{ - 0.02}^{ + 0.02}$ 0.300.04+0.07$0.30_{ - 0.04}^{ + 0.07}$
rcav 1.60.9+1.0$1.6_{ - 0.9}^{ + 1.0}$ 4.21.2+0.5$4.2_{ - 1.2}^{ + 0.5}$ au

ɀ0 205.260.9+59.3$205.2_{ - 60.9}^{ + 59.3}$ 24.73.7+23.9$24.7_{ - 3.7}^{ + 23.9}$ au Fsky 6.560.05+0.05$6.56_{ - 0.05}^{ + 0.05}$ 1.420.03+0.04$1.42_{ - 0.03}^{ + 0.04}$ mJy km s−1
ψ 1.560.13+0.10$1.56_{ - 0.13}^{ + 0.10}$ 0.600.09+0.15$0.60_{ - 0.09}^{ + 0.15}$ Fcorr 9.680.38+0.46$9.68_{ - 0.38}^{ + 0.46}$ 1.590.07+0.10$1.59_{ - 0.07}^{ + 0.10}$ mJy km s−1
ϕ 0.870.10+0.15$0.87_{ - 0.10}^{ + 0.15}$ 19.1518.08+27.57$19.15_{ - 18.08}^{ + 27.57}$

If 0.420.03+0.02$0.42_{ - 0.03}^{ + 0.02}$ 0.090.01+0.02$0.09_{ - 0.01}^{ + 0.02}$ mJy/px R68% 131.21.8+1.9$131.2_{ - 1.8}^{ + 1.9}$ 72.44.3+3.8$72.4_{ - 4.3}^{ + 3.8}$ au
αf 0.320.01+0.03$0.32_{ - 0.01}^{ + 0.03}$ 0.800.11+0.05$0.80_{ - 0.11}^{ + 0.05}$ R90% 182.33.0+3.0$182.3_{ - 3.0}^{ + 3.0}$ 94.68.2+8.7$94.6_{ - 8.2}^{ + 8.7}$ au
βf 2.580.11+0.13$2.58_{ - 0.11}^{ + 0.13}$ 15.7411.26+3.76$15.74_{ - 11.26}^{ + 3.76}$ R95% 203.63.3+3.2$203.6_{ - 3.3}^{ + 3.2}$ 102.210.7+11.9$102.2_{ - 10.7}^{ + 11.9}$ au

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