Fig. 6
M2–M1 diagram for V479 And. The solution probably lies between thick diagonal lines corresponding to q = 0.54 and 0.7 as measured by RV amplitude ratio of He ii and Hβ emission lines to the absorption. Dashed curves denote the orbital inclination of the system. The shaded area corresponds to the mass range of a K0 star from ZAMS to luminosity class IV.
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