Query= WZ Sge GCVS Query forms
  NNo      GCVS          J2000.0            Type      Max        Min I         Min II       Epoch        Year      Period          M-m/D     Spectrum      References  Other desig. p.m.(as/yr)   Epoch     Ident.     New type    GCVS
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710048 |WZ    Sge *|200736.46 +174214.7 |UGSU+E+ZZ |  7.0    |  15.53     |            |B |            |     |(11900.           ) |     |DAep(UG)         |09709 09472|           |             |1992.741| |GSC2.2   |          |WZ    Sge |
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_______________Cross-identifications:_______________
WZ    Sge     = EG   136                      |     
WZ    Sge     = HV   03518                    |     
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      Reference to a chart or photograph:
09472. G.Williams, ApJ Suppl 53, N3, 523, 1983.

Reference to a study of the star:
09709. M.F.Walker, M.Bell, ApJ 237, 89, 1980.

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Remark: Nova Sge 1913, 1946, 1978. VB A (B 15.76m B, 7", 280deg). Really it is not a nova. Three outbursts were registered up to day: JD2420094, 32001, 43844 [09710, 09711]. There are superhumps on the light curve during the outburst with 0.057250d >= P >= 0.05714d (A=0.3m V) [09710, 09776]. There are light variations between the outbursts (A = 0.14m - 0.3m). During some of light weakenings Algol-like eclipses are observed (A = 0.2m) with the elements: Min I = 2437547.72845 + 0.0566878455d*E [09774]; D = 0.04P. d = 0.02P. There are also rapid light oscillations (A <= 0.01m). The periods of these oscillations before the 1978 outburst were 28.98s and 27.87s [09774], but after this outburst - 28.95963s [09775]. According to [09777], in 1976 - 78 these oscillations were represented by the elements: Max = 2443311.790250 + 0.00032254826d*E + 9.8d*10**(-16)*E**2.

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