Velocity-resolved high-J CO emission from massive star-forming clumps

Open Access

Fig. 4

Fraction of the integrated emission in the line wings of CO 11−10 (left) and CO 16−15 (right), as a function of L_bol /M_clump (Table 1). Dashed horizontal lines show the mean wing fraction at each evolutionary stage. The colour-coding is the same as in Fig. 3.

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