Improving 1D stellar atmosphere models with insights from multidimensional simulations - II. 1D versus 3D model comparison for Wolf-Rayet stars

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Table 2

Stellar parameters for the β-law and modified hydrodynamical PoWR models to match the profile of Moens et al. (2022a).

Model	log(L_⋆/L_⊙)	$\log (\dot{M} / M_{⊙} {yr}^{- 1})$ $\log \,(\dot{M}/{{M}_{\odot }}\text{y}{{\text{r}}^{-1}})$	v_∞ (10³ km s ⁻¹)	log T_eff (K)	M_⋆/M_⊙	v_Dop (km s ⁻¹)	Framework
Γ2	5.47	–4.82	0.62	4.70	10	100	$\begin{array}{l} β = 1 \\ {PoWR}_{M}^{HD} \end{array}$ $\begin{array}{*{35}{l}} \,\,\,\beta =1 \\ \text{PoWR}_{\text{M}}^{\text{HD}} \\\end{array}$
Γ2	5.47	–4.82	0.65	4.70	11.3	100
Γ3	5.64	–4.49	1.05	4.70	10	100	$\begin{array}{l} β = 1 \\ {PoWR}_{M}^{HD} \end{array}$ $\begin{array}{*{35}{l}} \,\,\,\,\beta =1 \\ \text{PoWR}_{\text{M}}^{\text{HD}} \\\end{array}$
Γ3	5.64	–4.50	1.58	4.81	11.3	100
Γ3	5.56	–4.50	1.32	4.73	10	100	${PoWR}_{L}^{HD}$ $\text{PoWR}_{\text{L}}^{\text{HD}}$
Γ3	5.64	–4.41	1.43	4.74	10	50	${PoWR}_{v}^{HD}$ $\text{PoWR}_{\text{v}}^{\text{HD}}$
Γ4	5.74	–4.14	1.35	4.61	10	100	$\begin{array}{l} β = 1 \\ {PoWR}_{M}^{HD} \end{array}$ $\begin{array}{*{35}{l}} \,\,\,\beta =1 \\ \text{PoWR}_{\text{M}}^{\text{HD}} \\\end{array}$
Γ4	5.74	–4.12	1.82	4.66	10.2	100
Γ4	5.72	–4.12	1.77	4.65	10	100	${PoWR}_{L}^{HD}$ $\text{PoWR}_{\text{L}}^{\text{HD}}$
Γ4	5.74	–4.13	1.63	4.65	10	50	${PoWR}_{v}^{HD}$ $\text{PoWR}_{\text{v}}^{\text{HD}}$

Notes. All fundamental parameters are scaled at τ = 2/3. All the models have a v_turb = 21 km s⁻¹.

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