Fig. 9
Line-wing ratios of 12CO J = 10–9/J = 3–2 as a function of absolute offset from the source velocity for the sources NGC 2071 (top) and W3-IRS5 (bottom) for the red and blue wings. The shaded regions are obtained from the average spectra of the low-mass sample for these transitions (see Yıldız et al. 2013). The spectra have been resampled to 0.6 km s-1 bin and shifted to 0 km s-1.
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