Fig. 10.
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Predicted stellar Hβ absorption line strength EW(Hβ) vs a measure of Balmer Break. The red, blue, and magenta triangles show the A2, A4, and B3 SMS models, respectively. The SSP models with an age range of 0.1 Myr–15 Gyr are shown with the red line. Models of individual main sequence stars with log g = 4.5 and varying Teff are shown as dots color-coded according to temperature.
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