Merging of a CO WD and a He-rich WD to produce a type Ia supernovae

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Fig. 4

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Similar to Fig. 3, but for the delay-time distributions of SNe Ia. The open square is from Graur & Maoz (2013), the filled triangles and squares are from Maoz et al. (2010, 2012), and the open circles are taken from Totani et al. (2008).

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