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Table 3.
Intermediate polars used by Pretorius & Mukai (2014) to obtain the space density.
| Name | D̃ (pc) |
|
fX (erg cm−2 s−1) | p (mas) | Δp (mas) | log LX (s−1) | D (pc) | Dmax (pc) | Vgen (pc3) |
|---|---|---|---|---|---|---|---|---|---|
| V1223 Sgr | 527 | 33.6 | 1.18E–10 | 1.725 | 0.047 | 33.7 | 571 | 1241 | 1.22E+09 |
| V2400 Oph | 280 | 32.7 | 5.00E–11 | 1.399 | 0.033 | 33.5 | 701 | 991 | 1.51E+09 |
| AO Psc | 330 | 32.6 | 3.20E–11 | 2.021 | 0.043 | 33.0 | 488 | 552 | 5.48E+07 |
| IGR J16500 | 430 | 32.8 | 2.60E–11 | 0.855 | 0.062 | 33.6 | 1140 | 1163 | 2.46E+09 |
| V405 Aur | 380 | 32.8 | 3.50E–11 | 1.487 | 0.031 | 33.3 | 662 | 783 | 5.78E+08 |
| FO Aqr | 450 | 33.1 | 5.20E–11 | 1.902 | 0.051 | 33.2 | 518 | 747 | 7.76E+07 |
| PQ Gem | 510 | 33.0 | 3.10E–11 | 1.306 | 0.036 | 33.3 | 750 | 835 | 4.28E+08 |
| TV Col | 368 | 33.0 | 6.00E–11 | 1.951 | 0.018 | 33.3 | 505 | 782 | 1.94E+08 |
| IGR J15094 | 960 | 33.5 | 2.60E–11 | 0.859 | 0.028 | 33.6 | 1127 | 1149 | 2.35E+09 |
| XY Ari | 270 | 32.5 | 3.60E–11 | 3.700 | 1.500 | 32.5 | 270 | 324 | 4.33E+07 |
| EI UMa | 750 | 33.3 | 2.90E–11 | 0.883 | 0.037 | 33.6 | 1095 | 1179 | 1.66E+08 |
| NY Lup | 680 | 33.7 | 9.20E–11 | 0.786 | 0.028 | 34.2 | 1228 | 2356 | 9.38E+09 |
| V1062 Tau | 1400 | 33.8 | 2.50E–11 | 0.632 | 0.077 | 33.8 | 1512 | 1512 | 2.72E+09 |
| V2731 Oph | 1000 | 33.9 | 6.90E–11 | 0.436 | 0.056 | 34.6 | 2165 | 3597 | 2.25E+09 |
| GK Per | 477 | 33.3 | 7.80E–11 | 2.263 | 0.043 | 33.3 | 437 | 772 | 7.74E+08 |
Notes. The luminosity is given in the spectral band 14–195 keV. Distances and luminosities with tildes are from the orginal publication, those without are from this work. Vgen was computed for a scale height of 120 pc.
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