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

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Table B.1

S CrA N continuum compensated pure Brγ line visibilities.

PBL	PA	^a	^a	^b	^b	^c	^c
[m]	[°]

42	53	0.98±0.02	1.00±0.02	1.00±0.03	1.00±0.03	1.00±0.03	1.00±0.03
52	38	0.99±0.01	1.00±0.02	1.00±0.02	1.00±0.02	1.00±0.02	1.00±0.02
60	130	0.89±0.02	0.92±0.03	0.99±0.02	1.00±0.03	0.91±0.03	0.96±0.03
81	100	0.88±0.02	0.98±0.03	0.98±0.02	1.00±0.03	0.90±0.02	1.00±0.04
93	45	0.83±0.01	0.90±0.02	0.93±0.02	1.00±0.02	0.86±0.02	0.95±0.02
115	76	0.85±0.01	0.80±0.02	0.94±0.02	0.89±0.02	0.89±0.02	0.85±0.02

Notes.

^(a)

Averaged continuum compensated pure Brγ visibilities over three spectral channels at ~–34 km s^-1 () and ~+75 km s^-1 ().

^(b)

As a but computed assuming a decrease of the line flux of 10% with respect to the measured one.

^(c)

As a but computed assuming an increase of the continuum flux of 10% with respect to the measured one.

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