Fig. 6
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CO spectra averaged over the full survey fields. L 1622 and Ori B9 each show two distinct velocity components, L1641-S also features a double peaked spectrum, while the NGC 2023, NGC 2024, NGC 2068, and NGC 2068 areas show single peaked spectra, though a hint of a secondary component is seen as a blue shoulder in the NGC 2023 & NGC 2024 spectra.
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