The wind and the magnetospheric accretion onto the T Tauri star S Coronae Australis at sub-au resolution

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Table 3

Geometric Gaussian fitting: pure Brγ line visibilities.

	Single-parameter fit		Three-parameter fit
RV		a ^a		a ^a	i	PA^b
[km s^-1]		[mas]		[mas]	[°]	[°]

–71	1.96	0.49 ± 0.04	2.51	0.63 ± 0.16	32	162 ± 19
–35	2.03	0.51 ± 0.03	2.09	0.66 ± 0.14	31	168 ± 15
3	1.45	0.54 ± 0.03	2.54	0.54 ± 0.07	40	153 ± 44
39	0.60	0.48 ± 0.03	0.92	0.47 ± 0.04	38	77 ± 48
75	2.12	0.46 ± 0.04	2.92	0.46 ± 0.05	32	85 ± 31
112	2.38	0.47 ± 0.06	3.39	0.47 ± 0.07	29	77 ± 36

Notes. Single and three-parameter fit of pure Brγ line visibilities at different radial velocities (RV).

^(a)

Size of the semimajor axis.

^(b)

Position Angle of the semimajor axis with North up and East to the left.

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