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Table 2.

Summary of models.

Models ϵ w Pm Pk Pth θout vmax
(LEdd) (LEdd/c2) (LEdd/c) (LEdd) (LEdd) (c)
(1) (2) (3) (4) (5) (6) (7) (8)
A1 0.1 3.90×10−2 4.53×10−4 2.66×10−5 1.94×10−7 14.9°-24.0° 0.046
A2 0.2 4.95×10−1 1.67×10−2 2.86×10−3 4.19×10−6 21.2°-50.6° 0.114
A3 0.3 6.27×10−1 2.86×10−2 6.54×10−3 5.75×10−6 24.0°-55.5° 0.188
A4 0.4 6.16×10−1 3.08×10−2 7.90×10−3 6.59×10−6 25.6°-55.5° 0.186
A5 0.5 9.21×10−1 4.30×10−2 1.06×10−2 1.08×10−5 24.8°-66.6° 0.176
A6 0.6 1.58 1.28×10−1 5.47×10−2 1.52×10−6 28.1°-42.1° 0.484
A7 0.7 1.83 1.73×10−1 8.18×10−2 7.95×10−7 28.1°-43.4° 0.438
A8 0.8 1.95 2.75×10−1 2.08×10−1 9.76×10−5 28.1°-57.3° 0.563

B1 0.1 / / / / / /
B2 0.2 4.76×10−2 6.34×10−4 4.46×10−5 2.22×10−7 10.1°-27.2° 0.042
B3 0.3 2.37×10−1 6.67×10−3 9.55×10−4 1.31×10−6 16.5°-36.0° 0.107
B4 0.4 3.55×10−1 1.38×10−2 2.74×10−3 1.71×10−6 15.4°-43.4° 0.146
B5 0.5 8.54×10−1 3.07×10−2 5.57×10−3 9.09×10−6 18.7°-32.8° 0.146
B6 0.6 8.98×10−1 5.76×10−2 1.90×10−2 1.80×10−6 24.8°-31.8° 0.341
B7 0.7 1.23 5.88×10−2 1.50×10−2 4.71×10−6 17.0°-28.1° 0.334
B8 0.8 1.30 8.70×10−2 2.92×10−2 2.64×10−7 18.1°-30.9° 0.401

C1 0.1 / / / / / /
C2 0.2 5.37×10−2 7.89×10−4 5.83×10−5 1.21×10−7 12.3°-20.5° 0.051
C3 0.3 1.79×10−1 3.37×10−3 3.20×10−4 6.95×10−7 13.1°-34.9° 0.073
C4 0.4 3.40×10−1 1.08×10−2 1.75×10−3 1.38×10−6 17.0°-42.1° 0.129
C5 0.5 4.41×10−1 1.68×10−2 3.14×10−3 1.49×10−6 15.9°-43.4° 0.136
C6 0.6 4.45×10−1 1.75×10−2 3.49×10−3 2.39×10−6 18.1°-46.2° 0.142
C7 0.7 5.60×10−1 1.21×10−2 1.67×10−3 2.41×10−6 14.0°-26.4° 0.131
C8 0.8 1.26 3.31×10−2 6.17×10−3 3.54×10−6 17.5°-24.0° 0.210

Notes. Column (1): run names; Column (2): the ratio of disc luminosity to Eddington luminosity; Column (3): the time-averaged values of the mass outflow rate; Column (4)-(6): the time-averaged values of the momentum flux, the kinetic flux, and thermal energy flux, which are carried out by winds at the outer boundary; Column (7): the azimuth range of winds at the outer boundary; Column (8): the maximum speed of winds. Runs A1–A8 ignore the special relativity effects caused by disc rotation and gas motion. The A-group runs is identical to the models proposed by Proga et al. (2000). Runs B1–B8 take into account the special relativity effect caused by disc rotation but ignore the radiation-drag term in equation (6). Runs C1–C8 take into account the special relativity effect caused by disc rotation and the radiation-drag effect.

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