A biconical ionised gas outflow and evidence of positive feedback in NGC 7172 uncovered by MIRI/JWST

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Table 1.

Flux measurements of the main neon emission lines (R = 0.5″).

Line	IP	f_AGN	f_NE	f_SW	f_C1
	(eV)	(×10⁻¹⁶ erg s⁻¹ cm⁻²)
[Ne II]	21.6	238.07 ± 0.65	8.86 ± 0.30	12.58 ± 0.34	8.40 ± 0.05
[Ne III]	41.0	377.35 ± 0.64	7.07 ± 0.34	12.82 ± 0.14	5.68 ± 0.09
[Ne V]	97.2	294.25 ± 0.58	4.19 ± 0.28	4.20 ± 0.11	1.94 ± 0.07
[Ne VI]	126.0	40.12 ± 1.76	4.23 ± 0.30	2.47 ± 0.19	–

Notes. The regions of interest are described in Sect. 3 and shown in Fig. 1. All the fluxes have been estimated using a single Gaussian modelling. We have not applied an aperture correction.

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