The outflow of gas from the Centaurus A circumnuclear disk - Atomic spectral line maps from Herschel/PACS and APEX

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Table 2

Spectral lines observed with Herschel/PACS.

Line	Wavelength	Ionisation	Beam^b	Spectral resolution^b
		potentials^a	FWHM	wavelength	velocity
	(μm)	(eV)	(′′)	(μm)	( km s^-1)

[N III]	57.317	29.60–47.45	9.5	0.021	108
[O I]	63.184	– 13.62	9.5	0.017	88
[O III]	88.356	35.12–54.94	9.5	0.034	124
[N II]	121.898	14.53–29.60	10	0.116	300
[O I]	145.525	– 13.62	11	0.123	255
[C II]	157.741	11.26–24.38	11.5	0.126	240
[N II]	205.178	14.53–29.60	16	0.102	150

Notes.

^(a)

Potentials required for creation and ionisation of the species, respectively.

^(b)

Taken from on-line PACS Observer’s Manual, version 2.4.

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