Table 5.
Mass transfer rates determined by fitting the SED of each system using a model consisting of a white dwarf plus steady-state accretion disc model.
| Source | Period | log10 (Ṁ | ± | Ṁ | ± |
|---|---|---|---|---|---|
| (mins) | (M⊙ yr−1) | (M⊙ yr−1) | |||
| ES Cet | 10.4 | −7.61 | 0.46 | 2.5 × 10−8 | 1.6 × 10−8 |
| SDSSJ1351 | 15.7 | −8.58 | 1.13 | 2.6 × 10−9 | 2.4 × 10−9 |
| SDSSJ1908 | 18.1 | −6.18 | 0.27 | 6.6 × 10−7 | 3.1 × 10−7 |
| HP Lib | 18.4 | −8.26 | 0.19 | 5.5 × 10−9 | 1.9 × 10−9 |
| ASASSN-14cc | 22.5 | −8.63 | 0.14 | 2.3 × 10−9 | 6.5 × 10−10 |
| ASASSN-14mv | 41.0 | −8.59 | 0.16 | 2.6 × 10−9 | 7.9 × 10−10 |
| ASASSN-14ei | 43.0 | −10.14 | 0.13 | 7.2 × 10−11 | 1.9 × 10−11 |
| SDSSJ1525 | 44.3 | −10.15 | 0.46 | 7.1 × 10−11 | 4.6 × 10−11 |
| SDSSJ1411 | 46.0 | −10.44 | 0.17 | 3.6 × 10−11 | 1.2 × 10−11 |
| GP Com | 46.6 | −10.64 | 0.25 | 2.3 × 10−11 | 1.0 × 10−11 |
| Gaia14aae | 49.7 | −10.48 | 0.06 | 3.3 × 10−11 | 4.3 × 10−12 |
| SDSSJ1208 | 53.0 | −11.15 | 0.15 | 7.1 × 10−12 | 2.1 × 10−12 |
| SDSSJ1137 | 59.6 | −11.09 | 0.28 | 8.1 × 10−12 | 3.9 × 10−12 |
| V396 Hya | 65.1 | −10.86 | 0.26 | 1.4 × 10−11 | 6.2 × 10−12 |
| SDSSJ1319 | 65.6 | −10.94 | 0.26 | 1.1 × 10−11 | 5.2 × 10−12 |
Notes. Apart from the eclipsing system (Gaia14aae), we fixed the mass of the white dwarf at M1 = 0.8 ± 0.1 M⊙ and cos(i) = 0.5. We varied radius of the accretion disc to achieve a good fit. The large error the mass transfer rate of SDSS J1505 is due to the large error on the distance.
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