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Table 6
Relative fluxes (in percentages) from the different emission components of J2256.
| Parameter/Set | B 1 | B 2 | V 1 | V 2 | R 1 | R 2 | I 1 | I 2 |
|
|
||||||||
| * F max,total | 37.1 | 35.6 | 27.5 | 26.0 | 18.7 | 19.4 | 12.0 | 13.7 |
|
|
||||||||
| White dwarf | ||||||||
| Fmin(ϕ = 0.0) | 0.0 | 0.0 | 0.0 | 0.0 | ||||
| ** ϕ ecl | 0.0435 | 0.0466 | 0.0495 | 0.0460 | ||||
| F max | 5.3 | 5.5 | 3.6 | 3.7 | 2.4 | 2.3 | 1.5 | 1.3 |
| Secondary star | ||||||||
| Fmin(ϕ = 0.0) | 0.6 | 1.8 | 2.7 | 2.5 | 7.1 | 7.3 | 13.1 | 13.1 |
| Fmax(ϕ = 0.5) | 10.1 | 20.3 | 15.2 | 22.5 | 25.5 | 27.7 | 33.2 | 33.1 |
| Quadratures | 11.1 | 21.5 | 16.8 | 24.6 | 28.6 | 31.5 | 37.4 | 36.9 |
| Disk with hot spot | ||||||||
| Fmin(ϕ =0 .0) | 0.2 | 0.2 | 0.1 | 0.1 | 0.2 | 0.0 | 0.0 | 0.7 |
| ⟨ Fplato ⟩(ϕ ~ 0.1−0.6) | 72.0 | 66.6 | 75.6 | 68.8 | 61.5 | 56.7 | 56.7 | 56.9 |
| Orbital hump (ϕ ~0.8) | 76.5 | 72.2 | 80.0 | 75.8 | 64.2 | 62.9 | 57.5 | 64.2 |
| Hot line | ||||||||
| Fmin(ϕ = 0.0) | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 |
| Fmax(ϕ = 0.2) | 9.4 | 7.3 | 5.8 | 4.6 | 9.6 | 8.2 | 6.7 | 5.8 |
| Fmax(ϕ = 0.8) | 17.3 | 19.9 | 13.1 | 15.8 | 17.6 | 17.0 | 16.7 | 12.4 |
| ** ϕ ecl | 0.103 | 0.109 | 0.099 | 0.106 | 0.082 | 0.078 | 0.085 | 0.098 |
Notes. *Fmax,total is in conditional units; *ϕecl is the orbital phase of the appearing of the corresponding component after its eclipse.
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