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

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Table 4

Comparison between the observed and predicted peak intensities and velocity peak-to-peak separations for Hnα RRLs toward MWC349A assuming a central mass of 38 M_⊙.

Line	ν	S _{blue peak,obs}	S _{red peak,obs}	S _peak,pred	(v_red − v_blue)_obs	(v_red − v_blue)_pred
	[GHz]	[Jy]	[Jy]	[Jy]	[km s^-1]	[km s^-1]

H39α	106.74	0.75^a	0.7^a	0.7	~34^b	30.5 ± 0.1
H36α	135.29	1.1^c	1.5^c	1.2	36.5 ± 0.4^a	35.8 ± 0.5
H35α	147.05	1.18 ± 0.07^a	2.48 ± 0.07^a	1.5	38.5 ± 0.5^b	36.4 ± 0.5
H30α	231.90	24.4^c	38.9^c	19.1	51.0 ± 0.1^a	51.0 ± 0.1
H27α	316.42	25.6 ± 0.6^a	34.4 ± 0.4^a	137	52.5 ± 0.1^a	54.4 ± 0.1
H26α	353.62	39.7 ± 0.4^a	60.0 ± 0.6^a	873	51.8 ± 0.1^a	58.2 ± 0.1
H21α	662.40	309 ± 11^c	261 ± 11^c	~10¹⁴	50.1 ± 0.4^c	90.0 ± 0.4

Notes.

^(a)

Thum et al. (1995).

^(b)

Martín-Pintado et al. (1994).

^(c)

Thum et al. (1994b).

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