Table 2
Break frequencies, disk truncation radii, and time delays of the dwarf novae analyzed in this work.
Source | State | Break Freq. (mHz) | Radius (× 109 cm) | Delay (s) | Log(LUVW1/LX) |
|
|||||
SS Cyg | (quiescence-XMM) | 5.6 ± 1.4 | 4.8 ± 1.2 | 166–181 (![]() |
–4.3 |
SS Cyg | (quiescence-RXTE) | 4.5 ± 1.3 | 5.5 ± 1.8 | ||
SS Cyg | (X-ray Dips) | 50.0 ± 20.0 | 1.1 ± 0.5 | ||
SS Cyg | (X-ray peak) | 9.7 ± 1.5 | 3.3 ± 0.5 | ||
RU Peg | (quiescence) | 2.8 ± 0.5 | 8.2 ± 1.5 | 97–109 (![]() |
–3.1 |
VW Hyi | (quiescence) | 2.0 ± 0.6 | 8.1 ± 2.5 | 103–165 (![]() |
–2.7 |
WW Cet | (quiescence) | 3.0 ± 1.7 | 6.8 ± 3.8 | 118–136 (![]() |
–3.6 |
T Leo | (quiescence) | 4.5 ± 1.5 | 4.0 ± 1.3 | 96–121 (![]() |
–3.7 |
Notes. The last column is the logarithm of the ratio between the UV and X-ray luminosities. The UV luminosities are in erg s-1 Å-1 obtained using the XMM-Newton OM UVW1 filter. The errors represent 90% confidence level. The values are for the delays calculated from fits with the subtracted CCFs except for SS Cyg for which a single Lorentzian fit was applied.
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