**Table C.1:** The difference between the integrated CO( $J\rightarrow J-1$ ) intensities from the best-fit model and the observations, in percent; $(I_{\rm {mod}}-I_{\rm {obs}})/I_{\rm {obs}}$ .
Source	OSO	JCMT
	$1\rightarrow0$		$2 \rightarrow 1$	$3 \rightarrow 2$	$4\rightarrow 3$	$6\rightarrow 5$
LP And	3.2		5.4	15.8	4.2	-0.6
CW Leo	4.8		-7.3	-15.6	-11.7	$\cdots$
RW LMi	-16.6		37.4	-1.6	6.2	$\cdots$
V384 Per	-22.3		-20.3	63.8	-15.3	$\cdots$
AFGL 3068	6.3		-4.2	11.0	-13.3	34.6
TX Cam	-7.7		56.9	40.2	-18.9	$\cdots$
GX Mon	1.6		-3.4	-1.9	3.4	$\cdots$
WX Psc	-3.2		-14.8	23.8	6.8	273.7
IK Tau	-3.3		-1.4	9.2	16.4	$\cdots$
IRC-10529	-3.5		-44.8	11.9	38.9	$\cdots$

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