Re: more on WX Hyi's peculiar superoutburst(s)


Fraser Farrell wrote ( vsnet-obs 4520):

> Our complete observations of  the peculiar superoutburst of WX Hyi  during
> October-November.  After looking at the lightcurve with VSSPlot 2.0b I'm
> beginning to wonder if this star is trying to become a UGZ, or just
> redefining the meaning of UGSS !
> 
> 
> November observations
> WX HYI       2450391.9396  <13.7       Tz
> WX HYI       2450393.9368   12.4       Tz
> WX HYI       2450393.9569   12.4       Tz
> WX HYI       2450394.9924   13.0       MKA
> WX HYI       2450400.9535  <12.5       MKA
> WX HYI       2450405.9444   12.8       MKA
> WX HYI       2450410.0465   13.0       Tz
> WX HYI       2450413.9444  <13.0       Tz
> 
> October observations (previously reported)
> WX HYI       2450359.9382  <13.7       Tz
> WX HYI       2450363.0535   12.0       Tz
> WX HYI       2450363.9326   11.3       Tz
> WX HYI       2450364.0014   11.7       MKA
> WX HYI       2450365.9264   11.1       Tz
> WX HYI       2450366.9201   11.8       MKA
> WX HYI       2450369.0576   12.0       MKA
> WX HYI       2450369.9625   11.3       Tz
> WX HYI       2450370.0104   12.0       MKA
> WX HYI       2450370.9514   11.7       Tz
> WX HYI       2450373.0160   12.4       MKA
> WX HYI       2450373.9521   12.4       Tz
> WX HYI       2450376.9500  <13.7       Tz
> WX HYI       2450377.9708  <12.6       MKA
> WX HYI       2450379.9646   12.5       Tz
> WX HYI       2450386.9417   12.4       Tz
> WX HYI       2450386.9514   12.3       Tz
> WX HYI       2450386.9632   12.5       Tz
> WX HYI       2450386.9722   12.2       Tz
> WX HYI       2450386.9819   12.2       Tz
> WX HYI       2450386.9868   12.5       Tz
> WX HYI       2450386.9910   12.5       Tz
> 
> MKA = Michael Mattiazzo, 20cm Newtonian (light-polluted site)
> Tz = Justin Tilbrook, 20cm Newtonian

SU UMa-type dwarf novae tend to redefine themselves in the northern hemisphere. We know four well-observed members of a peculiar group of ever-erupting (Z Cam-like) SU UMa-type dwarf novae called ER UMa stars or RZ LMi stars. The group presently consists of ER UMa, V1159 Ori, RZ LMi and DI UMa. They all show extremely short outburst cycle lengths of 3-4 days, recurrence time of superoutbursts of 19-44 days. Is WX Hyi wishing to join this group?

References:

Discovery and observations of ER UMa stars or RZ LMi stars:

  Kato T., Kunjaya C. 1995, PASJ 47, 163
  Robertson J. W., Honeycutt R. K., Turner G. W. 1995, PASP 107, 443
  Misselt K. A., Shafter A. W. 1995, AJ 109, 1757
  Nogami D., Kato T., Masuda S., Hirata R. 1995a, IBVS No.4155
  Nogami D., Kato T., Masuda S., Hirata R., Matsumoto K., Tanabe K.,
       Yokoo T. 1995b, PASJ 47, 897
  Patterson J., Jablonski F. Coen C., O'Donoghue D., Skillman D. R.
       1995, PASP 107, 1183
  Warner B. 1995, ApSS, 226, 187 (review on SU UMa stars)

Theory:

  Osaki Y. 1995a, PASJ 47, L11
  Osaki Y. 1995b, PASJ 47, L25
  Osaki Y. 1996, PASP 108, 39 (review on dwarf nova outbursts)

Regards,
Taichi Kato


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