The formation and stability of a cold disc made out of stellar winds in the Galactic centre

Open Access

Fig. 10

Synthetic X-ray spectra computed from the numerical models in an annulus of 0.5″ < p < 1.5″. The models WR_f07 and WR_f1 are shown in solid orange and dashed blue lines, respectively. Additionally, the thin solid black line corresponds to the results from the SPH model (Balakrishnan et al. 2024b).

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