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Table 2.
Non-magnetic CVs used by Pretorius & Knigge (2012) to obtain the space density of RASS-selected objects.
| RBS# | Name | D̃ (pc) |
|
fX (erg cm−2 s−1) | p (mas) | Δp (mas) | log LX (s−1) | D (pc) | Dmax (pc) | Vgen (pc3) |
|---|---|---|---|---|---|---|---|---|---|---|
| 2 | EF Tuc | 346 | 31.4 | 1.60E–12 | 0.720 | 0.023 | 32.5 | 1335 | 1610 | 4.25E+08 |
| 22 | WW Cet | 158 | 31.2 | 5.70E–12 | 4.588 | 0.047 | 31.5 | 216 | 492 | 6.84E+07 |
| 280 | TT Ari | 335 | 31.7 | 3.50E–12 | 3.884 | 0.070 | 31.4 | 256 | 457 | 8.16E+07 |
| 288 | WX Hyi | 260 | 31.4 | 3.00E–12 | 4.273 | 0.029 | 31.3 | 232 | 383 | 5.03E+07 |
| 372 | IQ Eri | 116 | 30.4 | 1.20E–12 | 5.186 | 0.167 | 30.7 | 192 | 201 | 1.01E+07 |
| 490 | 285 | 31.2 | 1.60E–12 | 3.098 | 0.126 | 31.3 | 320 | 386 | 5.42E+07 | |
| 512 | VW Hyi | 64 | 30.5 | 6.10E–12 | 18.531 | 0.022 | 30.3 | 54 | 127 | 3.40E+06 |
| 664 | TW Pic | 230 | 31.0 | 1.70E–12 | 2.284 | 0.022 | 31.6 | 432 | 537 | 1.42E+08 |
| 694 | SU UMA | 261 | 31.9 | 9.00E–12 | 4.535 | 0.029 | 31.7 | 219 | 626 | 1.97E+08 |
| 710 | SW UMa | 164 | 30.6 | 1.40E–12 | 6.148 | 0.080 | 30.6 | 162 | 183 | 9.24E+06 |
| 728 | BZ UMa | 228 | 31.1 | 2.30E–12 | 6.557 | 0.064 | 30.8 | 152 | 220 | 1.49E+07 |
| 1008 | T Leo | 101 | 30.6 | 3.60E–12 | 7.814 | 0.069 | 30.8 | 128 | 232 | 1.45E+07 |
| 1411 | RHS40 | 468 | 31.6 | 1.90E–12 | 2.919 | 0.671 | 31.5 | 367 | 482 | 6.92E+07 |
| 1900 | TY PsA | 239 | 31.3 | 2.80E–12 | 5.431 | 0.065 | 31.1 | 183 | 292 | 2.48E+07 |
| 1955 | V405 Peg | 149 | 30.5 | 1.20E–12 | 5.784 | 0.062 | 30.6 | 172 | 179 | 8.92E+06 |
| 1969 | CC Scl | 359 | 31.4 | 1.50E–12 | 4.904 | 0.148 | 30.9 | 203 | 237 | 1.48E+07 |
| NEP1 | EX Dra | 240 | 29.7 | 8.10E–14 | 4.058 | 0.019 | 29.8 | 244 | 491 | 4.93E+05 |
| NEP2 | RXJ1831 | 980 | 31.5 | 2.80E–13 | 1.232 | 0.038 | 31.3 | 793 | 2967 | 8.60E+06 |
| NEP3 | SDSSJ1730 | 444 | 31.2 | 7.30E–13 | 1.864 | 0.038 | 31.4 | 528 | 3190 | 5.08E+06 |
| NEP4 | RXJ1715 | 400 | 30.4 | 1.20E–13 | 1.382 | 0.146 | 30.9 | 713 | 1747 | 3.64E+06 |
Notes. The luminosity is given in the spectral band 0.5–2.0 keV. Distances and luminosities with tildes are from the original publication, those without are from this work. Vgen was computed for a scale height of 260 pc.
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