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Table 13
Summary of known and candidate cataclysmic variables in our two fields.
Name | Src-ID | Type | B (mag) | Comment |
(USNO) | ||||
|
||||
IR Com | Com141a | SU | 13.4 | |
J1238+1946 | – | WD | 17.4 | 1 |
S10980 Com | Com101a | 18.5 | 2 | |
DO Vul | – | SU | 20.7 | |
J1953+1859 | – | SU | 20.4 | |
V458 Vul | – | Nova | 3 | |
QQ Vul | Sge21a | AM | 14.4 | |
V405 Vul | Sge40a | SU | 19.0 | |
WZ Sge | Sge80a | SU | 15.0 | |
HM Sge | Sge102a | Nova | ||
S11015 Vul | Sge33a | 14.8 | ||
S11017 Vul | Sge42a | 15.5 | ||
S11020 Vul | Sge48e | 18.6 | 2 | |
Sge48h | AM | 17.2 | ||
S11035 Vul | Sge92e | 17.8 | ||
S11029 Vul | Sge114f | 16.3 | 4 | |
S11030 Vul | Sge115b | 14.6 | 2 | |
S11038 Aql | Sge120a | IP | 17.2 | |
S11033 Aql | Sge130b | 17.6 |
Notes. (1) WD = white dwarf. Double-degenerate binary (Brown et al. 2013). (2) Is not the counterpart of the X-ray source. (3) ROSAT observation was prior to outburst of 2007. (4) Is possibly not the counterpart of the X-ray source.
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