Table 6.
Updated list of CVs with anomalously warm secondary according to Wakamatsu et al. (2021) and El-Badry et al. (2021) with orbital periods ≤5 hours.
System | Period | G | Distance | Spec. Type | Ref. |
---|---|---|---|---|---|
[h] | [mag] | [pc] | Secondary | ||
KSP-OT-201712a | 0.97 | 17.7 | 1400(130) | K4.5 ± 0.5 | 1 |
V485 Cen | 0.98 | 17.9 | 331(7) | K8 | 2 |
EI Psc | 1.07 | 15.9 | 149(1) | K4 ± 2 | 3 |
QZ Ser | 2.00 | 17.3 | 320 | K4 ± 2 | 4 |
CzeV404 Her* | 2.35 | 15.9 | 340 | K7 ± 1 | 5 |
V1239 Her | 2.40 | 17.8 | 440 ± 30 | M0 ± 0.5 | 6 |
SDSS J001153.08−064739.2 | 2.41 | 17.2 | 484 | K4 ± 3 | 7 |
CSS J134052.0+151341 | 2.45 | 18.0 | 790? | K4 ± 2 | 8 |
ASAS-SN 18aan | 3.58 | 16.8 | 675(+32/−29) | G9 | 9 |
ASAS-SN 13cl* | 4.86 | 17.7 | – | K4 ± 2, | 10 |
V1460 Her* | 4.99 | 15.0 | 263 | K5, | 11 |
ASAS-SN 15cm | 5.00 | 18.7 | – | K2.5 ± 2.5 | 12 |
Notes. 1 – Lee et al. (2024), 2 – Politano (2004), 3 – This paper, 4 – Thorstensen et al. (2002b), 5 – Kára et al. (2021), 6 – Littlefair et al. (2006), 7 – Rebassa-Mansergas et al. (2014), 8 – Thorstensen (2013), 9 – Wakamatsu et al. (2021), 10 – Thorstensen (2015), 11 – Ashley et al. (2020), 12 – Thorstensen et al. (2016). * – eclipsing system.
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