Fig. 10.
Colors for Galactic DPVs (Mennickent et al. 2016), Be stars (Howells et al. 2001), and synthetic stellar atmosphere models with log g = 4.0 (squares with lines) and log g = 3.0 (open circles with lines) from Bessell et al. (1998). The effective temperature of two selected synthetic models have been labeled along with the position of UU Cas.
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