Table 2.
Results of the SED fit.
| Model | Teff sdB | R sdB | Teff disc | R disc | E(B − V) |
|---|---|---|---|---|---|
| (K) | (R⊙) | (K) | (R⊙) | ||
| TMAP & Kurucz | 23 000 ± 3000 | 0.12 ± 0.04 | 6000 ± 1800 | 0.30 ± 0.05 | 0.04 ± 0.03 |
| TMAP & Black body | 21 000 ± 3000 | 0.15 ± 0.04 | 5000 ± 1500 | 0.33 ± 0.05 | 0.05 ± 0.03 |
Notes. The top line gives the results of the fit performed with the TMAP models in combination with the Kurucz models used to model the circumstellar matter, while in the bottom line the circumstellar matter is modeled by a black body. In the table, the parameters for the circumstellar matter are marked with ‘disc’.
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