Table 4
Cataclysmic variables with blackbody-like soft X-ray emission and fast spinning white dwarfs.
Source | Other name | Periods | kT [eV] | Comment | References |
|
|||||
RX J0512.2-3241 | UU Col | 863.5 s/3.45 h | 50 | soft IP | 3, 12, 13 |
RX J0558.0+5353 | V 405 Aur | 545.5 s/4.15 h | 57 | soft IP | 2, 4, 13 |
1RXS J062518.2+733433 | MU Cam | 1187 s/4.72 h | ~43 | soft IP? | 8 |
1RXS J070407.9+262501 | V 418 Gem | 480 s/4.37 h | 85 | soft IP | 14, 15 |
1E 0830.9-2238 | WX Pyx | 1557.3 s/~5.54 h | 82 | soft IP | 10, 13 |
RE 0751+14 | PQ Gem | 833.7 s/5.19 h | 52 | soft IP | 1, 2, 5, 13 |
1RXS J154814.5-452845 | NY Lup | 693.0 s/9.87 | ~100 | soft/hard IP | 7, 11, 13 |
1RXS J180340.0+401214 | V 1323 Her | 1520.5 s/4.4 h | 100 | soft IP | 14 |
RX J0806.3+1527 | HM Cnc | 321.5 s | 65 | double degenerate | 9, 16 |
RX J1914.4+2456 | V 407 Vul | 567.7 s | 43 | double degenerate | 2, 6 |
3XMM J051034.6−670353 | 1418 s | 69 | double degenerate? | this work |
Reference. 1) Mason et al. (1992); 2) Haberl & Motch (1995); 3) Burwitz et al. (1996); 4) Skillman (1996); 5) Hellier (1997); 6) Cropper et al. (1998); 7) Haberl et al. (2002); 8) Staude et al. (2003); 9) Israel et al. (2003); 10) Schlegel (2005); 11) de Martino et al. (2006a); 12) de Martino et al. (2006b); 13) Evans & Hellier (2007); 14) Anzolin et al. (2008); 15) Patterson et al. (2011); 16) Esposito et al. (2014).
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