Physical structure and water line spectrum predictions of the intermediate mass protostar OMC2-FIR4

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Table 1:

Range of the input parameters to DUSTY covered in the present study.
Parameter	Range
$\alpha$	0.2-3.9
Y	100-2200
$\tau _{100}$	0.1-4.6
$T_{\rm in}$	300 K
T_*	5000 K

The range of the $\alpha$ , Y and $\tau _{100}$ parameters is covered by increasing their respective value at each step of the grid by 20%. Note that $T_{\rm in}$ and T_* are kept fixed because they do not influence the results (see text).

Source LaTeX | All tables | In the text

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