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Table 1.

Main characteristics of the detached stage of systems with a solar composition donor star of M2, i = 1.25 M and a MNS, i = 1.3 M.

Porb, i/d T/Gyr Δt/Myr M2/M MNS/M Log10(L/L) Log10(Teff/K) Porb/d R2/RL
1.00 6.210 200 0.2170 2.1016 0.4691 3.7070 3.2396 0.868
1.20 5.703 108 0.2515 2.0773 0.6129 3.6713 4.6738 0.898
1.44 5.561 93 0.2677 2.0649 0.6674 3.6644 5.2709 0.897
1.72 5.479 82 0.2851 2.0518 0.7129 3.6589 5.7044 0.901
2.07 5.366 69 0.3139 2.0292 0.7942 3.6525 6.5564 0.900
2.48 5.312 59 0.3554 1.9581 0.8473 3.6488 7.0681 0.889
2.98 5.278 48 0.4050 1.8970 0.9167 3.6465 7.5675 0.890
3.58 5.256 42 0.4511 1.8432 0.9970 3.6451 8.6100 0.869
4.29 5.255 35 0.5067 1.8009 1.0704 3.6445 9.1894 0.873
5.15 5.253 29 0.5658 1.7376 1.1533 3.6441 9.9515 0.878
6.19 5.256 24 0.6212 1.6759 1.2381 3.6432 10.9982 0.881
7.43 5.260 20 0.6598 1.6213 1.3349 3.6404 12.8373 0.880
8.91 5.263 16 0.7203 1.5524 1.4098 3.6397 14.1156 0.875
10.69 5.268 13 0.7857 1.4841 1.4915 3.6385 15.5098 0.878
12.83 5.270 12 0.9633 1.3953 1.5519 3.6439 14.2132 0.900

Notes. The first column gives the initial orbital period. The second column gives the age of the system in the middle of the detached stage. The third column gives the time spent in the detached state. The fourth and fifth columns present the masses of the donor and NS at the Huntsman regime, respectively. The rest of the columns give the luminosity, the effective temperature, the orbital period, and the filling factor, all of them evaluated in the middle of the detached stage.

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