Name |
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CF | ![]() |
F3-100 | F0.1- 100 | ![]() |
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d | ![]() |
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1022 cm-2 | 1016 g s-1 | erg s-1 | pc | |||||
V1223 Sgr |
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1.0a | ![]() |
4.2 | 7.3 | 12.6 | 24.3 | 5271 | 105.4(63) |
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FO Aqr |
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1.5 | 4.9 | 10.2 | 9.4 | 4002 | 62.1(65) |
EX Hya |
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1.0 | ![]() |
1.5 | 3.4 | 0.25 | 0.17 | 64.53 | 85.3(65) |
AO Psc |
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1.3 | 2.5 | 4.7 | 4.9 | 4204 | 55.8(65) |
TVCol |
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1.7 | 3.5 | 3.4 | 5.7 | 3685 | 63.4(65) |
GK Per |
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1.0a | ![]() |
12.5 | 88.6 | 81.5 | 156 | 3406 | 110.5(63) |
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V709 Cas |
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2.3 | 3.7 | 5.76 | 11.1 | (500) | 56.3(65) |
PQ Gem |
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1.0 | ![]() |
0.80 | 1.3 | 3.7 | 3.9 | (500) | 38.7(65) |
V2400 Oph |
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2.43 | 5.6 | 18.7 | 16.75 | (500) | 78.5(65) |
BG CMi |
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0.77 | 1.54 | 5.3 | 9.0 | 7007 | 57.4(65) |
V405 Aur |
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0.9 | 1.7 | 2.65 | 5.09 | (500) | 51.6(65) |
V1062 Tau |
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1.1 | 1.8 | 2.2 | 5.4 | 5008 | 45.6(65) |
DO Dra |
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7.8 | 14.4 | 3.1 | 4.1 | 1559 | 69.7(65) |
TX Col |
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<0.4 | <60 | 0.32 | 0.58 | 1.8 | 2.1 | 55010 | 52.6(65) |
a - For the systems V1223 Sgr and GK Per which have very
high mass accretion rates we used two absorbers.
References to distance estimates: 1. Beuermann et al. (2004); 2. McHardy et al. (1987); 3. Beuermann et al. (2003); 4. Hellier et al. (1991); 5. McArthur et al. (2001); 6. Warner (1987); 7. Berriman (1987); 8. Szkody & Silber (1996); 9. Mateo et al. (1991); 10. Buckley & Tuohy (1989). |