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Table 1

Sonic point properties of our set of chemically homogeneous helium star models with a mass of 15 M (see Sect. 4).

log ( ) RS log (L) κ log (ρS ) log (TS ) log (λ) v Γ t log (HP) log (Teff) τS
M∕yr R L cm2/g g/cm3 K cm km/s cm K

–4.3 1.152 5.464 0.658 –7.971 5.331 8.125 36.55 0.9901 8.097 9.218 5.099 33
–4.5 1.158 5.466 0.659 –8.165 5.312 8.350 35.73 0.9918 6.689 9.335 5.097 20
–4.7 1.165 5.467 0.660 –8.359 5.291 8.521 34.91 0.9931 5.754 9.451 5.096 13
–5.0 1.182 5.469 0.661 –8.656 5.259 8.827 33.62 0.9946 4.708 9.628 5.093 8
–5.1 1.190 5.468 0.661 –8.753 5.246 8.921 33.14 0.9952 4.787 9.680 5.091 6
–5.3 1.216 5.469 0.661 –8.959 5.212 9.133 31.87 0.9964 5.790 9.768 5.087 3
–5.4 1.260 5.470 0.626 –8.843 4.726 8.985 18.20 0.8978 0.138 7.827 5.079 2
Same as above, but for our set of models with a mass of 10 M

log () RS log (L) κ log (ρS) log (TS) log (λ) v Γ t log (HP) log (Teff) τS

M∕yr R L cm2/g g/cm3 K cm km/s cm K

–4.3 0.910 5.115 0.986 –7.748 5.295 7.748 35.03 0.9828 9.766 8.832 5.061 49
–4.5 0.914 5.120 0.979 –7.937 5.267 7.937 33.93 0.9861 8.418 8.908 5.061 28
–4.7 0.920 5.123 0.971 –8.118 5.221 8.118 32.17 0.9883 13.29 8.909 5.061 16
–5.0 0.930 5.136 0.842 –8.225 4.814 8.225 20.13 0.8173 0.625 7.565 5.061 8
–5.1 0.930 5.136 0.846 –8.311 4.791 8.311 19.62 0.8082 0.523 7.556 5.061 6
–5.3 0.931 5.136 0.855 –8.493 4.747 8.493 18.64 0.7866 0.377 7.544 5.061 3
Same as above, but for our set of models with a mass of 20 M

log () RS log (L) κ log (ρS) log (TS) log (λ) v Γ t log (HP) log (Teff) τS

M∕yr R L cm2/g g/cm3 K cm km/s cm K

–4.3 1.362 5.678 0.545 –8.123 5.344 8.376 37.09 0.9934 5.158 9.438 5.114 27
–4.5 1.371 5.679 0.544 –8.320 5.327 8.597 36.37 0.9945 4.213 9.571 5.113 18
–4.7 1.383 5.680 0.543 –8.517 5.310 8.775 35.68 0.9954 3.635 9.707 5.111 11
–5.0 1.409 5.681 0.542 –8.821 5.283 9.081 34.58 0.9963 2.931 9.917 5.108 6
–5.1 1.421 5.681 0.542 –8.921 5.274 9.182 34.23 0.9965 2.731 9.988 5.106 2
–5.3 1.453 5.682 0.542 –9.135 5.255 9.398 33.48 0.9971 2.487 10.14 5.101 1

Notes. The listed quantities are, starting from the left: mass-loss rate applied, sonic point radius, luminosity, Rosseland opacity, density, temperature, photon mean free path, flow velocity, Eddington factor, optical depth parameter, pressure scale height, effective temperaturecomputed via the Stefan–Boltzmann law, optical depth. All these quantities are given at the sonic point.

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