Self-generated ultraviolet radiation in molecular shock waves - II. CH+ and the interpretation of emission from shock ensembles

Open Access

Fig. 14

Lyα contribution to the UV flux escaping the shock front for shocks with magnetic parameter b = 1 and no external radiation field, G₀ = 0. Top: flux relative to the Mathis ISRF, with flux equal to the standard ISRF at the 0 contour. Bottom: flux relative to the kinetic flux of the shock as a percentage.

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