Dynamically inflated wind models of classical Wolf-Rayet stars

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Table 5

Summary of derived parameters of our steady-state and time-dependent models.

Model	Ṁ	v_∞	R_ph	T_{ph, eff}
	(M_⊙ yr⁻¹)	(km s⁻¹)	R_⊙	kK
Steady-state	1.47 × 10⁻⁵	2200	4.48	62
Time-dependent	1.64 × 10⁻⁵	2063	4.64	60

Notes. Listed are mass-loss rate, terminal velocity, radius of photosphere, and effective temperature at photosphere.

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