Mass of accreted matter as a function of the time needed to spin-up the progenitor NS to the observed properties of PSR J1614−2230 (i.e., M, B, and f) for the five models indicated in Table 3. The dot corresponds to a spin-up track proceeding at a rate equal to the Eddington accretion rate ṀEdd ~ 3 × 10-8M⊙/ yr; the accretion timescale is then ~2 Myr. For tracks with τacc ≲ 2 Myr, Ṁ is greater than ṀEdd.
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