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Table 3

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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