ALMA captures feeding and feedback from the active galactic nucleus in NGC 613

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Table 4.

Gaussian fit in the nuclear spectrum.

Component	S_CO	Position	FWHM	S_peak
	(Jy km s⁻¹)	(km s⁻¹)	(km s⁻¹)	(mJy)
Core ^(a)	68.5 ± 1.1	−11.8 ± 0.4	107.2 ± 0.9	600

	S_CO	Velocity range		S_peak
	(Jy km s⁻¹)	(km s⁻¹)		(mJy)

INTEGRATED RESIDUAL WINGS

Blue	2.63 ± 0.8	[−400,−90]		21.8
Red	2.62 ± 0.9	[+80,+300]		24.9

INTEGRATED RESIDUAL WINGS

Blue	2.3 ± 0.8	[−400,120]	41.5 ^(b)
Red	2.3 ± 0.9	[+120,+300]	41.7 ^(b)

Notes.

^(a)

Results of the Gaussian fit for the main disk contribution of the nuclear spectrum extracted in a r = 0.28″ aperture shown in Fig. 15.

^(b)

In this case we assumed that S_peak is the maximum flux in the nuclear spectrum within the selected velocity range of the blue and red wings.

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