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Fig. 4


Comparison of the dynamical (open circles) and spectroscopic (filled circles) mass measurements for luminosity class I objects (supergiants) with the evolutionary masses. The shaded region between the solid lines shows the full range (mstart to mend) of evolutionary masses for the rotating solar metallicity models. The dashed lines mark the upper and lower mass ranges for the non-rotating solar metallicity models, while the dotted lines bracket the possible masses for the rotating LMC metallicity models and the dashed-dotted lines enclose the SMC metallicity models. Double encircled objects are located in the LMC.

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