Table 2: Intensities and ratio of the [Ne II]12.8 $\mu$ m and [Ne III]15.6 $\mu$ m for Arp 299. The values of [Ne II] were measured by Dudley (1999) and should be considered as upper limits as they may be contaminated by the 12.7 $\mu$ m PAH feature (see text).
I([Ne II]) I([Ne III])

Source ( $10^{-15}~{\rm W~m}^{-2}$ ) ( $10^{-15}~{\rm W~m}^{-2}$ ) $\frac{I([{\rm NeIII}])}{I([{\rm NeII}])}$

A <2 - -

B1 0.7 >1.3 $\geq$ 1.8

C 2.0 1.3 $\geq$ 0.65

C $^\prime$ <0.9 0.5 >0.55

**Table 2:** Intensities and ratio of the [Ne II]12.8 $\mu$ m and [Ne III]15.6 $\mu$ m for Arp 299. The values of [Ne II] were measured by Dudley (1999) and should be considered as upper limits as they may be contaminated by the 12.7 $\mu$ m PAH feature (see text).
	I([Ne II])	I([Ne III])
Source	( $10^{-15}~{\rm W~m}^{-2}$ )	( $10^{-15}~{\rm W~m}^{-2}$ )	$\frac{I([{\rm NeIII}])}{I([{\rm NeII}])}$
A	<2	-	-
B1	0.7	>1.3	$\geq$ 1.8
C	2.0	1.3	$\geq$ 0.65
C $^\prime$	<0.9	0.5	>0.55

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