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Table 5
Sizes (HWHM) of the emitting regions.
| Baseline m | Continuum |
Brγ
|
Pfund |
|||
|---|---|---|---|---|---|---|
| mas | au | mas | au | mas | au | |
| 60 | 3.00 ± 0.09 | 1.03 ± 0.03 | 1.22 ± 0.23 | 0.41 ± 0.08 | 1.7 ± 0.41 | 0.57 ± 0.14 |
| 101 | 3.40 ± 0.15 | 1.15 ± 0.05 | 1.11 ± 0.12 | 0.38 ± 0.04 | 1.16 ± 0.15 | 0.37 ± 0.06 |
| 130 | 1.80 ± 0.02 | 0.61 ± 0.006 | 1.00 ± 0.18 | 0.34 ± 0.06 | 0.89 ± 0.19 | 0.30 ± 0.06 |
Notes. An inclination of 56 ± 4° and a position angle of the major axis of the disc of 71 ± 7° (Borges Fernandes et al. 2011) were inputs in the 2D elongated Gaussian model. The continuum is corrected for the stellar contribution.
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