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Table 8
Masses and radii predicted by evolutionary models of Baraffe et al. (1998) and Chabrier et al. (2000) for the given age, Teff, and log g estimates of the SINFONI sources.
| Objet | Age | Predicted mass from Teff | Predicted radius from Teff | L/L⊙ | Predicted | Semi-empirical | |
| mass from L/L⊙ | radius | ||||||
| (Myr) | (MJup) | (RJup) | (MJup) | (RJup) | |||
|
|
|||||||
| 2M1207 A | 7.5–9.1 | 24 ± 5 | 2.4 |
– | – | – | |
| TWA 5B | 7.5–9.1 | 24 ± 5 | 2.4 |
– | – | – | |
| CT Cha b | 2 ± 2 | 30 |
2.6 |
||||
| DH Tau B | 0.5–10 | 15 |
2.6 |
– | – | – | |
| HR7329 B | 8-20 | 35 |
2.7 ± 0.2 | – | – | – | |
| TWA22 A | 8–34 | 75 |
3.4 |
– | – | – | |
| TWA22 B | 8–34 | 75 |
3.4 |
– | – | – | |
| 2M0141 | 10–40 | 13 |
1.5 ± 0.1 | – | – | – | |
| – | 11 |
1.5 |
– | – | – | ||
| GSC8047 B | 10–40 | 22 |
1.6 |
– | – | – | |
| USco CTIO 108 B | 3–11 | 16 |
2.0 ± 0.1 | –3.19 ± 0.05 | 10–15 | 1.6 ± 0.1 | |
| OTS 44 | 1–6 | 6 |
1.7 |
–2.90 ± 0.08 | 9–17 | 3.8 |
|
| KPNO Tau 4 | 0.5–10 | 4 |
2.0 |
–2.49 ± 0.01 | 15–27 | 6.1 |
|
| Cha 1109 | 1–6 | 7 |
1.7 |
–3.23 ± 0.03 | 5–13 | 2.4 |
|
| AB Pic b | 10–40 | 13 |
1.5 ± 0.1 | –3.74 ± 0.07 | 10–14 | 1.4 ± 0.2 | |
| 2M0345 | 300–600 | 75 |
1.11 ± 0.06 | –3.58 ± 0.03 | 55–73 | 0.9 ± 1 | |
| Gl 417B | 80–250 | 30 ± 10 | 1.2 ± 0.1 | –3.84 ± 0.03 | 23–37 | 1.3 ± 0.1 | |
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