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VbvAstE-001

Book Boris V. Vasiliev Astrophysics

40 N 35 30 10 9 8 7 6 5

40 N 35 30 10 9 8 7 6 5 4 3 2 1 A/Z 1.5 25 20 15 10 5 0 -2.0 -1.5 -1.0 -0.5 0.0 0.5 1.0 1.5 2.0 log M/Mo. Figure 5.1: The mass distribution of binary stars [10]. On abscissa, the logarithm of the star mass over the Sun mass is shown. Solid lines mark masses, which agree with selected values of A/Z from Eq.(5.26). 33

40 N 35 30 10 9 8 7 6 5 4 3 2 1 A/Z 1.5 25 20 15 10 5 0 -2.0 -1.5 -1.0 -0.5 0.0 0.5 1.0 1.5 2.0 binary stars close binary stars log M/Mo. Figure 5.2: The mass distribution of close binary stars [11]. On abscissa, the logarithm of the star mass over the Sun mass is shown. Solid lines mark masses, which agree with selected values of A/Z from Eq.(5.26). The binary star spectrum is shown for comparison. 34

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