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Table 1

Calculated relevant parameters of IMXBs with different initial orbital periods and donor-star masses.

Bs Md,i Porb,i Porb Age Md MNS q tr wind Rd Teff Yc
(G) (M) (d) (d) (Gyr) (M) (M) (M yr-1) (M yr-1) (R) (K)

300 1.6 1.51 0.787 1.83 0.488 1.62 0.30 2.5 × 10-8 1.0 × 10-7 1.29 4767 0.98
1.7 1.46 0.787 1.50 0.521 1.61 0.32 2.8 × 10-8 1.0 × 10-7 1.32 4786 0.98
1.8 1.28 0.787 1.24 0.511 1.63 0.31 2.9 × 10-8 1.0 × 10-7 1.32 4786 0.98
1.9 1.23 0.787 1.05 0.603 1.60 0.38 3.9 × 10-8 1.0 × 10-7 1.39 4897 0.98

1000 1.8 1.81 0.787 1.28 0.509 1.49 0.34 1.0 × 10-7 1.0 × 10-7 1.32 4862 0.98
1.9 1.58 0.787 1.08 0.459 1.50 0.31 0.9 × 10-7 1.0 × 10-7 1.27 4894 0.98
2.0 1.40 0.787 0.92 0.449 1.50 0.30 0.9 × 10-7 1.0 × 10-7 1.26 4953 0.98
2.1 1.33 0.787 0.80 0.496 1.49 0.33 1.0 × 10-7 1.0 × 10-7 1.30 4996 0.98

Notes. The meaning of the columns is as follows: the surface magnetic field, the initial donor-star mass, the initial orbital period, and the orbital period, the age, the donor-star mass, the neutron-star mass, the mass ratio, the mass-transfer rate, the wind-loss rate, the donor-star radius, the effective temperature, and the center He abundance when when the orbital period can fit the observed values of Sco X-1 in the period-increasing phase.

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