All Tables

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.