Coupling hydrodynamics with comoving frame radiative transfer - III. The Wind Regime of Early-Type B Hypergiants

Open Access

Fig. D.1

IUE spectra of ζ¹ Sco. The blue line is the observation, and the black line is our final PoWRHD model. The shaded area marks the interval of ±500 km s⁻¹ around the reference wavelength.

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