Fig. 6.
Mass fraction (flatest) involved in last burst event as a function of the look-back time to last episode of star formation (
), color-coded according to Δ(age) for models with ages smaller than the age of the Universe at redshift z = 0.55. flatest > 0.1 stands for ∼10% of models having a large fraction of mass involved in the burst, as detailed in Sect. 2.4.
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