A multi-ion non-equilibrium solver for ionised astrophysical plasmas with arbitrary elemental abundances

Open Access

Fig. 14.

Time evolution of luminosity for selected oxygen and nitrogen emission lines for the 1D wind-wind simulation in Sect. 4, calculated as described in Sect. 4.2. The forward shock leaves the domain at around 45 kyr, and the associated sharp drop in some line luminosities is therefore artificial.

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