Table 4
Summary of our calculations as described in Sect. 4.1.
System | Esec/erg | ΔEmin/Esec | ΔE/Esec | ΔE/Esec | ΔE/Esec | ΔEmin/Esec | δmin |
|
|||||||
Applegate (1992) | Tian et al. (2009) | This paper | |||||
|
|||||||
(see Eq. (5)) | (see Eq. (7)) | Const.dens. | Two-zone | Full model | |||
|
|||||||
HS 0705+6700 | 2.2 × 1039 | 6.7 | 7.3 | 3,300 | 140 | 140 | 0.73 |
HW Vir | 2.0 × 1040 | 4.9 | 6.0 | 720 | 108 | 104 | 0.72 |
NN Ser | 2.7 × 1039 | 3.2 | 3.3 | 1100 | 64 | 64 | 0.73 |
NSVS14256825 | 8.3 × 1038 | 5.3 | 5.4 | 3200 | 101 | 102 | 0.73 |
NY Vir | 1.4 × 1039 | 5.5 | 5.6 | 2800 | 106 | 106 | 0.73 |
HU Aqr | 1.4 × 1040 | 0.10 | 0.10 | 240 | 1.9 | 1.9 | 0.732 |
QS Vir | 3.0 × 1040 | 0.039 | 0.040 | 170 | 0.71 | 0.77 | 0.71 |
RR Cae | 5.2 × 1039 | 2.8 | 2.9 | 560 | 59 | 59 | 0.73 |
UZ For | 4.1 × 1039 | 0.14 | 0.15 | 360 | 2.7 | 2.7 | 0.73 |
DP Leo | 2.9 × 1039 | 0.021 | 0.021 | 150 | 0.38 | 0.38 | 0.74 |
V471 Tau | 2.0 × 1042 | 0.014 | 0.014 | 12 | 0.26 | 0.26 | 0.84 |
|
|||||||
RU Cnc | 5.7 × 1043 | 0.074 | 0.076 | 1.7 | – | – | – |
AW Her | 8.5 × 1042 | 608 | 618 | 270 | – | – | – |
HR 1099 | 3.7 × 1043 | 0.21 | 0.22 | 10 | – | 6.7 | 0.64 |
BX Dra | 3.5 × 1043 | 0.00016 | 0.00016 | 0.92 | 0.0029 | 0.056 | 0.52 |
SZ Psc | 9.9 × 1043 | 0.12 | 0.13 | 4.7 | – | 4.84 | 0.61 |
Notes. The ratios ΔEmin/Esec denote the energy required to drive an Applegate mechanism of the observed magntiude over the available energy produced by the secondary star. The parameter δmin denotes the ratio of core radius to secondary star radius for which the minimum energy is obtained in the numerical model. The dash denotes imaginary values implying that no physical solution exists, as discussed in Sects. 3.4 and 4.1.
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