Table 5
Masses, Teff, surface gravity, and radii estimated from hot-start evolutionary models.
| Model | Input | Mass | Teff | log g | Radius |
| (MJup) | (K) | log (cm s-2) | (RJup) | ||
|
|
|||||
| DUSTY | M J |
|
|
|
|
| DUSTY | M H |
|
|
|
|
| DUSTY | M K s |
|
|
|
|
| DUSTY | M L ′ |
|
|
|
|
| DUSTY | M NB |
|
|
|
|
| DUSTY | M M ′ |
|
|
|
|
| DUSTY | T eff |
|
n.a. |
|
|
| DUSTY | L / L⊙ |
|
|
|
|
| COND | M J |
|
|
|
|
| COND | M H |
|
|
|
|
| COND | M K s |
|
|
|
|
| COND | M L ′ |
|
|
|
|
| COND | M NB |
|
|
|
|
| COND | M M ′ |
|
|
|
|
| COND | T eff |
|
n.a. |
|
|
| COND | L / L⊙ |
|
|
|
|
|
|
|||||
| FM08/1s | M J | ≥ 7.7 | ≥ 1333 | – | – |
| FM08/1s | M H | ≥ 10 | ≥ 1554 | – | – |
| FM08/1s | M K s | >10 | >1400 | – | – |
| FM08/1s | M L ′ | >10 | >1400 | – | – |
| FM08/1s | M NB | >10 | >1400 | – | – |
| FM08/1s | M M ′ | >10 | >1400 | – | – |
| FM08 | T eff | ≥ 9.0 | n.a. | – | – |
| FM08 | L / L⊙ | ≥ 8.0 | ≥ 1496 | – | – |
| FM08/5s | M J | ≥ 9.6 | ≥ 1483 | – | – |
| FM08/5s | M H | ≥ 10 | >1554 | – | – |
| FM08/5s | M K s | >10 | >1400 | – | – |
| FM08/5s | M L ′ | >10 | >1400 | – | – |
| FM08/5s | M NB | ≥ 10 | ≥ 1400 | – | – |
| FM08/5s | M M ′ | >10 | >1400 | – | – |
|
|
|||||
| SB/cf1s | M J |
|
– |
|
|
| SB/cf1s | M H |
|
– |
|
|
| SB/cf1s | M L ′ | ≥ 10 | – | – | – |
| SB/cf3s | M J |
|
– |
|
|
| SB/cf3s | M H |
|
– |
|
|
| SB/cf3s | M L ′ | ≥ 10 | – | – | – |
| SB/hy1s | M J | ≥ 9.5 | – | – | – |
| SB/hy1s | M H |
|
– |
|
|
| SB/hy1s | T eff | ≥ 8.5 | n.a. | – | – |
| SB/hy1s | L / L⊙ | ≥ 8.2 | ≥ 1574 | – | – |
| SB/hy1s | M L ′ | ≥ 10 | – | – | – |
| SB/hy3s | M J | ≥ 9.9 | – | – | – |
| SB/hy3s | M H |
|
– |
|
|
| SB/hy3s | M L ′ | ≥ 10 | – | – | – |
Notes. FM08 stands for “Fortney and Marley 2008” models (Marley et al. 2007; Fortney et al. 2008). SB/cf1s, SB/cf3s, SB/hy1s, and SB/hy3s correspond to Spiegel & Burrows (2012) evolutionary models with solar-metallicity cloud-free atmospheres, 3× solar-metallicity cloud-free atmospheres, 1× solar-metallicity cloudy atmospheres, and 3× solar-metallicity cloudy atmospheres, respectively.
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