Shocks in the warm neutral medium - II. Origin of neutral carbon at high pressure

Open Access

Fig. 4

Column density spectrum of neutral carbon observed towards HD 210839 (from Table 4 of JT11). The column densities are derived over velocity intervals of 0.5 km s⁻¹. Each point along the spectrum is colour-coded according to the value of the f₂ column density ratio to highlight velocity components at different thermal pressures.

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