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Fig. 3.

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Results of our model for the number density of CO (solid), C and O (dashed), C+ and O+ (dotted), and CO+ (dash-dotted) as a function of distance in our Solar System. The exact shape of the radial profile depends on the heliopause location and geometry, which is not fully modelled in this paper. The assumptions behind this plot are described in Appendix F. We note that the neutral and ionized oxygen number densities are roughly superimposed onto those of carbon.

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