[vsnet-alert 11847] Re: OT J104411.4+211307 superhumps update

[Taichi Kato]

OT J104411.4+211307 superhumps update

   Josch Hambsch and Ian Miller have further reported observations
of this object (=CSS100217:104411+211307).
The mean superhump period since March 5 has been firmly established
as 0.06025(3) d, 1.9% longer than the period of early superhumps.
Whether this period represents the typical superhump period of this
object needs to be examined by further observations and analysis.
If this fractional excess is confirmed, the object may be more
analogous to SU UMa-type dwarf novae like BC UMa rather than
extreme WZ Sge-type objects.