Free Access
Table 2.
Best fit relative fluxes of the T Tau system from an MCMC fit of the kernel phase triple model to the VISIR-NEAR data.
| Filter | λ [μm] | Star | Rel. flux | σemp | Flux [Jy] |
|---|---|---|---|---|---|
| ARIII | 8.98 | N | 1.000 | 0 | 8.12 ± 0.13 |
| ARIII | 8.98 | Sa |
 |
0.02 | 4.34 ± 0.11 |
| ARIII | 8.98 | Sb |
 |
0.02 | 0.10 ± 0.08 |
| SIV_1 | 9.81 | N | 1.000 | 0 | 9.81 ± 0.16 |
| SIV_1 | 9.81 | Sa |
 |
0.02 | 2.68 ± 0.07 |
| SIV_1 | 9.81 | Sb |
 |
0.02 | 0.02 ± 0.05 |
| SIV_2 | 10.71 | N | 1.000 | 0 | 10.04 ± 0.19 |
| SIV_2 | 10.71 | Sa |
 |
0.02 | 4.05 ± 0.13 |
| SIV_2 | 10.71 | Sb |
 |
0.02 | 0.66 ± 0.10 |
| NEII | 12.80 | N |
 |
0.03 | 9.63 ± 0.43 |
| NEII | 12.80 | Sa | 1.000 | 0 | 10.64 ± 0.42 |
| NEII | 12.80 | Sb |
 |
0.03 | 1.23 ± 0.32 |
Notes. We also report an empirical uncertainty (σemp) for the relative fluxes (see Sect. 4.4) as well as the final photometry of T Tau N, Sa, and Sb in all filters.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.