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Fig. 10

image

Crux tangency emission spectra showing [C ii], H i, and 12CO emission plotted against velocity (VLSR). The spectra are averaged over the longitude range indicated. Note that the intensity scale is normalized to the peak emission within the velocity range. The corresponding 1–σ error bars are indicated in the [C ii] and 12CO spectra at VLSR = 50 km s-1. The tangent velocity is also marked. The dashed lines indicate the [C ii] excess beyond the tangent velocity and 12CO peak in the spectra.

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