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Fig. 14.
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DTDs of SNe Ia with different αCE. The open circles with error bars represent the observation SNe Ia rate from elliptical galaxies and galaxy clusters (Totani et al. 2008; Maoz et al. 2010, 2012; Graur & Maoz 2013). Black solid and red dashed lines are for Ge’s and polytropic models, respectively.
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