Table 1: Main parameters relevant for the spin evolution of isolated neutron stars with hyperons. The labels "infx'' mark the configurations for which the curve ${M}_{\rm B}(R_{\rm eq})_{f}$ has a point of inflexion. For $f_{\rm 1,infx}<f<f_{\rm 2,infx}$ (corresponding masses $M_{\rm B}^{\rm (1,infx)}$ and $M_{\rm B}^{\rm (2,infx)}$) ${\rm BB_{st}}$ exists. For $M_{\rm B}>M_{\rm B,max}^{\rm stat}$ we have also ${\rm BB_{ut}}$, which is the only BB phenomenon for ${M}_{\rm B}> M_{\rm B}^{\rm (2,infx)}$. For $f>f_{\rm K,flat}$and $M_{\rm B}>M_{\rm B}^{\rm (K,flat)}$, a star which is initially in the mass-shedding (Keplerian) state, spins-up as it looses angular momentum. The characteristic S-shape of J(f) is then impossible.
Parameter N1H1 N2H1 N1H2 N2H2
$M_{\rm B,max}^{\rm stat}~[M_{\odot}]$ 1.83 2.05 1.73 1.95
$f_{\rm 1,infx}$ [Hz] 860 880 880 910
$M_{\rm B}^{\rm (1,infx)}~[M_{\odot}]$ 1.808 1.91 1.73 1.81
$f_{\rm K,flat}$ [Hz] 1030 970 1050 930
$M_{\rm B}^{\rm (K,flat)}~ [M_{\odot}]$ 1.96 2.01 1.87 1.82
$f_{\rm 2,infx}$ [Hz] 1100 1320 1080 1380
$M_{\rm B}^{\rm (2,infx)} ~[M_{\odot}]$ 1.9 2.17 1.79 2.06


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