A non-LTE radiative transfer model to study ionized outflows and disks. The case of MWC349A

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Table 5

Comparison between the observed and predicted peak intensities for Hnβ RRLs toward MWC349A.

Line	ν	S _peak,obs ^a	S _{peak,LTE pred}	ΔS_peak^b	S _{peak, non−LTE pred}
	[GHz]	[mJy]	[mJy]	[mJy]	[mJy]

H48β	111.89	68 ± 10	52	1.5σ	96.7
H38β	222.01	171 ± 10	211	4.3σ	433
H33β	335.21	330 ± 50	456	2.6σ	981
H32β	366.65	~460 ± 40	535	2.0σ	1186

Notes.

^(a)

Thum et al. (1995).

^(b)

ΔS_{peak,LTE pred} ≡ S_{peak,
obs} − S_peak,pred. Their values are shown in units of the rms noise of the spectra, σ.

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