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Fig. 3
[C i] 1−0 and CO 6−5 lines observed towards DM Tau (black) and typical offset positions (red; + 30′′,0′′ for [C i], + 18′′, + 6′′ for CO). The [C i] line towards the source is single-peaked and narrower than CO 6−5. The spectra are binned to 0.4 km s-1 per channel.
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