Fig. 7

Normalized line profiles of carbon-bearing species, illustrating their different kinematics. The solid vertical line marks the source velocity of 11.4 km s-1. The short vertical dashed lines show the CH hyperfine components except the one the vlsr is centered on. No CASSIS model was made for CH, see text. The CII absorption at 11...15 km s-1 is an artefact due to contamination in the reference spectra. The dip in CI at ~10 km s-1 as also due to reference beam contamination.
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