Constraining the geometry of the gas surrounding a typical galaxy at z = 3.4 with Lyα polarization

Open Access

Fig. C.1.

Simulated spectra in the spherical geometry considering smooth (top) and clumpy (bottom) media. The black solid lines represent Gaussian functions with a width of σ = 150 km s⁻¹, corresponding to the intrinsic Lyα profile estimated using the wind model in Section 4.1.

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