Table 6: Integrated temperatures for both CO-bright components and for the disk of UGC 1347. Both components were assumed to be Gaussian. A disk flux contribution was taken into account in the determination of the source sizes. The central component is not resolved. The values for the total galaxy represent IRAM 30 m single-beam measurements centered on the galaxy. A comparison of the two CO(1-0) spectra can be found in Fig. 7.
FWHM ¹²CO(1-0) ¹²CO(2-1) ¹³CO(1-0)

$\Theta_{\rm {S,Obs}}$ $I_{\rm {CO}}$ I $_{\rm {CO}}$ $I_{\rm {CO}}$

[ $^{\prime \prime }$ ] [K km s^-1] [K km s^-1] [K km s^-1]

Nucleus <6.6 40.1 $\pm$ 1.3 8.4 $\pm$ 1.0

South. $\rm 8.5^{+1.4}_{-1.6}$ $\rm 24.1^{+5.5}_{-0.6}$ 4.0 $\pm$ 0.6

Total galaxy 18.9 4.6 $\pm$ 0.3 1.7 $\pm$ 0.3

**Table 6:** Integrated temperatures for both CO-bright components and for the disk of UGC 1347. Both components were assumed to be Gaussian. A disk flux contribution was taken into account in the determination of the source sizes. The central component is not resolved. The values for the total galaxy represent IRAM 30 m single-beam measurements centered on the galaxy. A comparison of the two CO(1-0) spectra can be found in Fig. 7.
	FWHM	¹²CO(1-0)	¹²CO(2-1)	¹³CO(1-0)
	$\Theta_{\rm {S,Obs}}$	$I_{\rm {CO}}$	I $_{\rm {CO}}$	$I_{\rm {CO}}$
	[ $^{\prime \prime }$ ]	[K km s^-1]	[K km s^-1]	[K km s^-1]
Nucleus	<6.6	40.1 $\pm$ 1.3	8.4 $\pm$ 1.0
South.	$\rm 8.5^{+1.4}_{-1.6}$	$\rm 24.1^{+5.5}_{-0.6}$	4.0 $\pm$ 0.6
Total galaxy	18.9	4.6 $\pm$ 0.3		1.7 $\pm$ 0.3

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