Inverse problem solution for A0620−00 in frame of the model with an HL (b).
| Parameter . | |$C\, 2015-2016$| . | |$J\, 2016$| . | |$K\, 2016$| . | |$C\, 2016-2017$| . | |$J\, 2017$| . | |$K\, 2017$| . |
|---|---|---|---|---|---|---|
| . | Passive state . | Active state . | ||||
| Accretion disc | ||||||
| αg | 0.670(1) | 0.705(1) | 0.749(1) | 0.483(1) | 0.553(4) | 0.600(8) |
| Tin, K | 192 555 | 219 275 | 231 570 | 71 140 | 94 445 | 92 505 |
| ±545 | ±580 | ±2 060 | ±435 | ±2 060 | ±4 300 | |
| Hotline | ||||||
| av/a0 | 0.024(1) | 0.024(1) | 0.02(1) | 0.027(1) | 0.025(2) | 0.027(3) |
| bv/a0 | 0.376(4) | 0.374(3) | 0.36(3) | 0.491(4) | 0.498(2) | 0.48(3) |
| T25, K | 7 535 | 7 710 | 7 200 | 8 645 | 19 650 | 47 205 |
| ±80 | ±235 | ±1 515 | ±195 | ±2 535 | ±5 465 | |
| T75, K | 10 595 | 11 105 | 11 120 | 7955 | 15 940 | 34 600 |
| ±150 | ±165 | ±1 090 | ±105 | ±720 | ±1 776 | |
| Hotspot | ||||||
| RHS/a0 | 0.046(1) | 0.26(1) | 0.39(1) | 0.2(1) | 0.13(9) | 0.2(2) |
| Fd/Fall | 0.280(2) | 0.287(4) | 0.268(6) | 0.360(2) | 0.290(1) | 0.216(5) |
| FHL/Fall | 0.099(6) | 0.040(3) | 0.024(2) | 0.155(3) | 0.211(5) | 0.268(7) |
| Fn/Fall | 0.379(6) | 0.326(5) | 0.292(6) | 0.515(4) | 0.501(5) | 0.484(8) |
| N | 32 | 18 | 13 | 16 | 17 | 15 |
| |$\chi ^2_{\textrm{N},\, 0.10}$| | 53.7 | 34.8 | 27.7 | 32.0 | 33.4 | 30.6 |
| χ2 | 60.0 | 37.1 | 68.7 | 104 | 121 | 179 |
| Parameter . | |$C\, 2015-2016$| . | |$J\, 2016$| . | |$K\, 2016$| . | |$C\, 2016-2017$| . | |$J\, 2017$| . | |$K\, 2017$| . |
|---|---|---|---|---|---|---|
| . | Passive state . | Active state . | ||||
| Accretion disc | ||||||
| αg | 0.670(1) | 0.705(1) | 0.749(1) | 0.483(1) | 0.553(4) | 0.600(8) |
| Tin, K | 192 555 | 219 275 | 231 570 | 71 140 | 94 445 | 92 505 |
| ±545 | ±580 | ±2 060 | ±435 | ±2 060 | ±4 300 | |
| Hotline | ||||||
| av/a0 | 0.024(1) | 0.024(1) | 0.02(1) | 0.027(1) | 0.025(2) | 0.027(3) |
| bv/a0 | 0.376(4) | 0.374(3) | 0.36(3) | 0.491(4) | 0.498(2) | 0.48(3) |
| T25, K | 7 535 | 7 710 | 7 200 | 8 645 | 19 650 | 47 205 |
| ±80 | ±235 | ±1 515 | ±195 | ±2 535 | ±5 465 | |
| T75, K | 10 595 | 11 105 | 11 120 | 7955 | 15 940 | 34 600 |
| ±150 | ±165 | ±1 090 | ±105 | ±720 | ±1 776 | |
| Hotspot | ||||||
| RHS/a0 | 0.046(1) | 0.26(1) | 0.39(1) | 0.2(1) | 0.13(9) | 0.2(2) |
| Fd/Fall | 0.280(2) | 0.287(4) | 0.268(6) | 0.360(2) | 0.290(1) | 0.216(5) |
| FHL/Fall | 0.099(6) | 0.040(3) | 0.024(2) | 0.155(3) | 0.211(5) | 0.268(7) |
| Fn/Fall | 0.379(6) | 0.326(5) | 0.292(6) | 0.515(4) | 0.501(5) | 0.484(8) |
| N | 32 | 18 | 13 | 16 | 17 | 15 |
| |$\chi ^2_{\textrm{N},\, 0.10}$| | 53.7 | 34.8 | 27.7 | 32.0 | 33.4 | 30.6 |
| χ2 | 60.0 | 37.1 | 68.7 | 104 | 121 | 179 |
Notes. Fd/Fall and FHL/Fall are the relative contributions of the disc with a hotspot and an HL, respectively, to the total light. On other parameters, see above, Table 2.
Inverse problem solution for A0620−00 in frame of the model with an HL (b).
| Parameter . | |$C\, 2015-2016$| . | |$J\, 2016$| . | |$K\, 2016$| . | |$C\, 2016-2017$| . | |$J\, 2017$| . | |$K\, 2017$| . |
|---|---|---|---|---|---|---|
| . | Passive state . | Active state . | ||||
| Accretion disc | ||||||
| αg | 0.670(1) | 0.705(1) | 0.749(1) | 0.483(1) | 0.553(4) | 0.600(8) |
| Tin, K | 192 555 | 219 275 | 231 570 | 71 140 | 94 445 | 92 505 |
| ±545 | ±580 | ±2 060 | ±435 | ±2 060 | ±4 300 | |
| Hotline | ||||||
| av/a0 | 0.024(1) | 0.024(1) | 0.02(1) | 0.027(1) | 0.025(2) | 0.027(3) |
| bv/a0 | 0.376(4) | 0.374(3) | 0.36(3) | 0.491(4) | 0.498(2) | 0.48(3) |
| T25, K | 7 535 | 7 710 | 7 200 | 8 645 | 19 650 | 47 205 |
| ±80 | ±235 | ±1 515 | ±195 | ±2 535 | ±5 465 | |
| T75, K | 10 595 | 11 105 | 11 120 | 7955 | 15 940 | 34 600 |
| ±150 | ±165 | ±1 090 | ±105 | ±720 | ±1 776 | |
| Hotspot | ||||||
| RHS/a0 | 0.046(1) | 0.26(1) | 0.39(1) | 0.2(1) | 0.13(9) | 0.2(2) |
| Fd/Fall | 0.280(2) | 0.287(4) | 0.268(6) | 0.360(2) | 0.290(1) | 0.216(5) |
| FHL/Fall | 0.099(6) | 0.040(3) | 0.024(2) | 0.155(3) | 0.211(5) | 0.268(7) |
| Fn/Fall | 0.379(6) | 0.326(5) | 0.292(6) | 0.515(4) | 0.501(5) | 0.484(8) |
| N | 32 | 18 | 13 | 16 | 17 | 15 |
| |$\chi ^2_{\textrm{N},\, 0.10}$| | 53.7 | 34.8 | 27.7 | 32.0 | 33.4 | 30.6 |
| χ2 | 60.0 | 37.1 | 68.7 | 104 | 121 | 179 |
| Parameter . | |$C\, 2015-2016$| . | |$J\, 2016$| . | |$K\, 2016$| . | |$C\, 2016-2017$| . | |$J\, 2017$| . | |$K\, 2017$| . |
|---|---|---|---|---|---|---|
| . | Passive state . | Active state . | ||||
| Accretion disc | ||||||
| αg | 0.670(1) | 0.705(1) | 0.749(1) | 0.483(1) | 0.553(4) | 0.600(8) |
| Tin, K | 192 555 | 219 275 | 231 570 | 71 140 | 94 445 | 92 505 |
| ±545 | ±580 | ±2 060 | ±435 | ±2 060 | ±4 300 | |
| Hotline | ||||||
| av/a0 | 0.024(1) | 0.024(1) | 0.02(1) | 0.027(1) | 0.025(2) | 0.027(3) |
| bv/a0 | 0.376(4) | 0.374(3) | 0.36(3) | 0.491(4) | 0.498(2) | 0.48(3) |
| T25, K | 7 535 | 7 710 | 7 200 | 8 645 | 19 650 | 47 205 |
| ±80 | ±235 | ±1 515 | ±195 | ±2 535 | ±5 465 | |
| T75, K | 10 595 | 11 105 | 11 120 | 7955 | 15 940 | 34 600 |
| ±150 | ±165 | ±1 090 | ±105 | ±720 | ±1 776 | |
| Hotspot | ||||||
| RHS/a0 | 0.046(1) | 0.26(1) | 0.39(1) | 0.2(1) | 0.13(9) | 0.2(2) |
| Fd/Fall | 0.280(2) | 0.287(4) | 0.268(6) | 0.360(2) | 0.290(1) | 0.216(5) |
| FHL/Fall | 0.099(6) | 0.040(3) | 0.024(2) | 0.155(3) | 0.211(5) | 0.268(7) |
| Fn/Fall | 0.379(6) | 0.326(5) | 0.292(6) | 0.515(4) | 0.501(5) | 0.484(8) |
| N | 32 | 18 | 13 | 16 | 17 | 15 |
| |$\chi ^2_{\textrm{N},\, 0.10}$| | 53.7 | 34.8 | 27.7 | 32.0 | 33.4 | 30.6 |
| χ2 | 60.0 | 37.1 | 68.7 | 104 | 121 | 179 |
Notes. Fd/Fall and FHL/Fall are the relative contributions of the disc with a hotspot and an HL, respectively, to the total light. On other parameters, see above, Table 2.
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