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Fig. 3

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The log trPorb plane. Dots – persistent AM CVn systems with known distances; asterisks – outbursting AM CVn systems with known distances; solid lines – the upper and lower critical limits tr: (1) for M1 = 1.0, Y = 1.0; (2) for M1 = 0.6, Y = 1.0; (3) for M1 = 1.0, Y = 0.96,Z = 0.04; (4) for M1 = 1.0, Y = 1.0; (5) for M1 = 0.6, Y = 1.0. (M1 – in solar units). Dotted lines: evolution models for AM CVns through the WD channel (kindly provided by Chris Deloye).

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