Outflowing shocked gas dominates the NIR H2 emission from the dual AGN NGC 6240

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Table 3.

Line fluxes measured from the fit.

Line	$F_{line}^{tot .}$ $Mathematical equation: $ F_\mathrm{{line}}^\mathrm{{tot.}} $$	$F_{line}^{rot .}$ $Mathematical equation: $ F_\mathrm{{line}}^\mathrm{{rot.}} $$	$F_{line}^{nonrot .}$ $Mathematical equation: $ F_\mathrm{{line}}^\mathrm{{nonrot.}} $$
	[[10⁻¹⁵ erg s⁻¹ cm⁻²]
Paα	71.1 ± 0.4	25.43 ± 0.16	45.6 ± 0.4
Paβ	30.5 ± 2.6	9.6 ± 0.3	20.9 ± 2.5
H₂ 1-0 S(1)	57.5 ± 0.9	19.7 ± 0.5	37.8 ± 0.7
H₂ 0-0 S(8)	16.2 ± 0.1	8.0 ± 0.1	8.2 ± 0.1
[Fe II] λ1.257 μm	55.9 ± 1.1	19.4 ± 0.3	36.5 ± 1.1
[Fe II] λ1.644 μm	55.9 ± 0.4	19.81 ± 0.19	36.1 ± 0.4

Notes. $F_{line}^{tot .}$ $Mathematical equation: $ F_\mathrm{{line}}^\mathrm{{tot.}} $$ is the total line flux, integrated across the whole FoV; $F_{line}^{rot .}$ $Mathematical equation: $ F_\mathrm{{line}}^\mathrm{{rot.}} $$ is the line flux measured in the rotating components; $F_{line}^{nonrot .}$ $Mathematical equation: $ F_\mathrm{{line}}^\mathrm{{nonrot.}} $$ is the sum of fluxes of the Gaussian components (one or two) that account for non-rotating motions.

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