Table 1: Parameters of the dust disk around HH 30 derived from the model fits of the continuum emission. q and p have been fixed (see Sect. 3). The error bars are the $1\sigma$ formal errors from the fit. For the scale-height, h(r) = h₁₀₀ $\times$ $(r/100~{\rm AU})^h$ using notations of Paper I, we assume hydrostatic equilibrium, so h=1.5 for q=0, and h₁₀₀ is derived from T₁₀₀.

Parameters Values

PA ( $^\circ$ ) $35 \pm 1$

i ( $^\circ$ ) $81 \pm 2$

$R^{\rm c}_{\rm in}$ (AU) $40 \pm 5$

$R^{\rm c}_{\rm out}$ (AU) $128 \pm 3$

T₁₀₀ (K) $9 \pm 3$

q 0, fixed

Parameters Values

$\Sigma_{100}$ (cm^-2) $2.2 \pm 0.2 \times 10^{23}$

p 0, fixed

h₁₀₀ (AU) $11 \pm 3$

h 1.5, fixed

$\beta$ $0.4\pm 0.1$

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