**Table 1:** Comparison between our dynamical masses and spectroscopic masses from Kudritzki et al. (2006). Observed mass-loss rates from the same paper are also listed and compared to values from the model tracks of Blöcker (1995). He 2-108 is classified as *wels*, the other three are non-emission-line stars.
Object	M [ $M_\odot$ ]		$T_{\rm eff}$ [10³ K]		$\log \dot M$ [ $M_\odot$ yr^-1]
	dyn.	spec.	dyn.	spec.	spec.	evol. tracks
Tc 1	0.59	0.81	32	34	-7.46	-7.91
He 2-108	0.57	0.63	32	34	-6.85	-8.16
IC 418	0.61	0.92	37	36	-7.43	-7.82
NGC 3242	0.61	0.63	79	75	-8.08	-7.86

Source LaTeX | All tables | In the text