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

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Table 2

Parameters derived from the best fit of the FT continuum data for both S CrA components (see Fig. 2).

SCrA	Sp.	T_eff	k_s	k_c	f_s	f_h	f_c	i	PA^a	a	a
	Type	[K]						[°]	[°]	[mas]	[au]

North	G0	5920	1.35	–3.73±1.27	0.30±0.04	0.06±0.01	0.64±0.04	28±3	0±6	0.83±0.04	0.108±0.005
South	K0	5280	1.25	–4.03±0.74	0.52±0.02	0.10±0.01	0.38±0.02	22±6	–2±12	0.70±0.04	0.090±0.005

Notes. See text for parameter definition. The reduced χ² values of the best fit model are 1.71 and 1.35 for the North and South component, respectively.

^(a)

The PA corresponds to the major axis of the disc with North up and East to the left.

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