**Table 4:** Clumping corrected mass loss rates for the stars in common between the present sample and the sample of Lang et al. (2005).
Star	$\log \frac{\dot{M}}{\sqrt{f}}$	$\log \dot{M}$ (Lang et al.)	$\log \dot{M}$ (Lang et al.) corrected
1	-4.20	-4.72	-4.80
2	-4.22	-4.72	-4.66
3	-4.10	-4.37	-4.47
4	-3.85	-4.72	-4.64
5	-4.14	-4.43	-4.44
6	-4.12	-3.65	-3.66
8	-4.00	-4.34	-4.27
18	-4.85	-4.72	-4.62

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