Table 2
Predictions for planetary masses and orbits in the post-common envelope systems marked by Zorotovic & Schreiber (2013) as candidates for planets.
| System | M 1,obs [M⊙] | M2 [M⊙] | MP [MJ] | rP [AU] | rP,cons [AU] |
|
|
|||||
| Detached sdB+MS/BD PCEBs | |||||
|
|
|||||
| HW Vir | 0.485 | 0.142 | 6.8 | 10.1 | 1.0 |
| HS 0705+6700 | 0.483 | 0.134 | 6.7 | 9.2 | 0.94 |
| HS 2231+2441 | 0.47 | 0.075 | 5.3 | 3.3 | 0.34 |
| NSVS14256825 | 0.46 | 0.21 | 7.5 | 21.9 | 2.2 |
| NY Vir | 0.459 | 0.122 | 6.2 | 8.5 | 0.87 |
|
|
|||||
| Detached WD+MS PCEBs | |||||
|
|
|||||
| NN Ser | 0.535 | 0.111 | 6.6 | 5.4 | 0.055 |
| V 471 Tau | 0.84 | 0.93 | 16.9 | 90.9 | 9.3 |
| QS Vir | 0.78 | 0.43 | 13.5 | 30.1 | 3.1 |
| RR Cae | 0.44 | 0.183 | 7.0 | 18.7 | 1.9 |
|
|
|||||
| CVs | |||||
|
|
|||||
| UZ For | 0.71 | 0.14 | 8.6 | 4.9 | 0.51 |
| HU Aqr | 0.80 | 0.18 | 6.3 | 10.2 | 0.64 |
| DP Leo1 | 1.2 | 0.14 | 12 | 1.8 | 0.19 |
| DP Leo2 | 0.6 | 0.09 | 6.6 | 3.0 | 0.30 |
Notes. We focus here on the most massive planet to form in a given system. M1,obs denotes the mass of the primary and M2 the mass of the companion. MP is the expected mass of the planet. While MP is independent of the parameter αL, the orbit depends on its value. We therefore give the value rP for our fiducial scenario (αL = 12.5) and a more conservative case rP,cons (αL = 4). For the system DP Leo, the index
refers to stellar masses as given by Pandel et al. (2002) and Beuermann et al. (2011), while
is based on the masses given by Schwope et al. (2002).
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