Fig. 6
Final magnetic field, Bf, versus initial gravitational mass, for a star with final parameters M = 1.67 M⊙ and the frequency f = 465 Hz, for APR, DH, and BM EOSs. The accretion rate is Ṁ = 10-10 M⊙/yr (solid curves) and Ṁ = 10-9 M⊙/yr (dashed curves). Scaling relation 
is fulfilled, i.e., dashed curves match the solid ones multiplied by 
(color online).
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