DUSTY modelling of the LMC carbon stars.
|Identifier||Lum.||MLRDUSTY||v exp,DUSTY||r gd||MLRscaled|
|(L⊙)||(M⊙ yr-1)||(km s-1)||(M⊙ yr-1)|
|IRAS 05506||17 700||2.0 ×10-5||19.3||133||1.6 ×10-5|
|IRAS 05125||15 500||2.4 ×10-5||19.4||541||4.0 ×10-5|
|ERO 0529379||5 600||2.9 ×10-5||17.5||504||4.5 ×10-5|
|ERO 0518117||9 500||4.3 ×10-5||7.5||142||3.6 ×10-5|
Notes. Columns 3 and 4 give the gas MLR and gas expansion velocity for a gas-to-dust ratio of 200. Column 5 gives the gas-to-dust ratio that makes the observed expansion velocity equal to the observed gas-to-dust ratio, and the last column lists the gas MLR for that gas-to-dust ratio.
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