Physical structure of the envelopes of intermediate-mass protostars

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Table 3:

Range of the input parameters to DUSTY covered in the present study.
Parameter	Range	Step
$\alpha$	0.2-2.5	0.1
Y	50-2000	10
$\tau _{100}$	0.1-10.	0.1
$T_{\rm in}$	300 K
T_*	5000 K

Notes. The range of the $\alpha$ , Y and $\tau _{100}$ parameters are covered by increasing by a constant value at each step of the grid reported in the third column. Note that $T_{\rm in}$ and T_{_*} remain fixed as they do not influence the results (see text).

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