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

Open Access

Table D.1

Line wing emission of CO 11−10 towards G351.16+0.7 using various envelope tracers.

Transition	S_int^(a) (K km s⁻¹)	(K)	(K)
C¹⁸O9−8	33.9	1.9	2.4
C¹⁸O6−5	35.4 (4%)	1.9 (0%)	2.6 (8%)
¹³CO 10−9	32.5 (4%)	1.8 (5%)	2.2 (8%)
¹³CO 6−5	23.5 (31%)	1.7 (11%)	1.1 (54%)

Notes. Numbers inside brackets show the difference with respect to wing parameters obtained using the C¹⁸O 9−8 transition (top row). ^(a)Total integrated intensity of both blue and red wings.

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