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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