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Table 3

Parameters of bounce-back candidates.

NN/object Porb V q M1 M2 i LC1 References
(days) (mag) (M) (M) (K) (°)

1. GW Lib* 0.0533 19.1 0.060 0.84 0.05 11 van Spaandonk et al. (2010)

2. SDSS1238 0.056 17.8 1.0  ≪ 0.09 12 000  ≥ 70 +q Zharikov et al. (2006)
3. V455 And* 0.0563 16.5 0.060  >M9 11 500 83 +q Araujo-Betancor et al. (2005)
4. AL Com* 0.0567 20.0 0.060 16 300 +q Patterson et al. (1996)
5. SDSS1035 0.057 18.7 0.055 0.94 0.05 10 100 83 Littlefair et al. (2008)
6. SDSS0804* 0.059 17.9 0.05 1.0(1) 0.05 12 000  ≥ 70 +q Zharikov et al. (2008)
7. EG Cnc* 0.060 18.8 0.035 12 300 +s Patterson et al. (1998)
8. RX1050-14 0.062 17.6  <0.055 13 000  <65 Mennickent et al. (2001)
9. GD552 0.0713 16.6  <0.052  <0.08 10 900  <60 Unda-Sanzana et al. (2008)
10. RE1255 0.083 19.0  <0.06  >0.9  <0.08 12 000  <5 Patterson et al. (2005)

11. SDSS1610** 0.0582 19.0 +q Mukadam et al. (2010)

Notes. 

(1)

Light curve (LC) features: “+” LC shows a double-hump during the orbital period; “s” – during superoutburst; “q” – during quiescence; “–” absence of double-humps in LC.

(*)

Objects that demonstrate WZ Sge-type superoutburst.

(**)

The mass ratio of SDSS1610 is not known, but the object shows similar observational characteristics to selected candidates and the double-humped light curve.

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