The R136 star cluster dissected with Hubble Space Telescope/STIS - III. The most massive stars and their clumped winds

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Table 3

Free parameters in the optical-only and optical + UV fits.

Fit	Free parameters	Results
Optical-only	T_eff, g, v_eq sin i, Ṁ, x_He, (n_N, β)	Table I.2
Optical+ UV (high S/N)	T_eff, g, Ṁ, β, v_∞, f_cl, v_cl,start, v_windturb, f_ic, f_vel, n_N, n_C,(n_O, x_He)	Tables A.1, A.3
Optical+ UV (low S/N)	T_eff, g, Ṁ, β v_∞, f_cl	Table A.2

Notes. Parameters in brackets are free only in a subset of the runs, see text. The last column contains for each fit a reference to the table where the best fit parameters are presented. Parameter names are defined in the text.

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