Table 3.
Bright and faint phase spectral parameters in 2005 for the model TBabs*pcfabs*(bbodyrad + constant*(apec + apec + gaussian)).
| Rev. | Fbb | RBB | CovFrac | Fpl | Fbb/Fpl | LX | Ṁ |
|---|---|---|---|---|---|---|---|
| [cgs] | [km] | [%] | [cgs] | [erg s−1] | [M⊙ yr−1] | ||
| Bright phase | |||||||
| 1027 | 6.7 ± 0.1 | 65 | 50 | 2.64 ± 0.06 | 3.4 | 5.1 × 1032 | 5.9 × 10−11 |
| 1028 | 19 ± 2 | 94 | 50 | 4.06 ± 0.14 | 4.7 | 12 × 1032 | 1.4 × 10−10 |
| 1030 | 26 ± 2 | 113 | 61 | 3.68 ± 0.09 | 7.0 | 15 × 1032 | 1.7 × 10−10 |
| 1031 | 33 ± 2 | 125 | 56 | 3.24 ± 0.07 | 10.1 | 19 × 1032 | 2.0 × 10−10 |
| Mean faint phase | |||||||
| – |
 |
6 | – |
 |
0.9 | ||
Notes. Flux units are given in 10−10 erg cm−2 s−1 and 10−12 ergs cm−2 s−1, for the bright and faint phases, respectively. The plasma flux Fpl is the sum of the bolometric fluxes of the cool and the hot components. CovFrac is the covering fraction of the partial covering absorber. The luminosity LX is the sum of the blackbody and the plasma components with L = ηπd2Fbol with geometry factors ηBB = 2 and ηpl = 3.3, respectively (Beuermann et al. 2012). The mass accretion rate was computed for a white dwarf with Mwd = 0.78 M⊙.
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