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Fig. 16

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Calculated X-ray emission produced by LECR ions with the spectral parameters s = 1.9, Emin = 10 MeV nucleon-1, and the escape path length Λ = 5 × 1024 cm-2, interacting in a gas cloud of metallicity Z = 1.7   Z (as obtained in Sect. 5). In panel a) the abundances of the accelerated heavy ions are in solar proportion, but with a metallicity enhancement factor relative to the solar system (SS) composition (see text) fmet = 1 (dashed curve) and fmet = 10 (solid and dotted curves). Panel b) same but for the CRS composition (see text). The dotted curves show the effect of photoelectric absorption on the X-ray spectra for a H column density of 1023 cm-2.

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