One of the criteria used by Taichi Kato in his paper is:
"the presence of early superhumps (reflecting the 2:1 resonance) and long or multiple rebrightenings are the best distinguishing properties of WZ Sge-type dwarf novae."
I suspect the reason for not including this star is that such early superhaumps have not been detected (yet)
We must continue to observe (when weather permits!!!!!!)
Kind regards
Stephen [HSP]
Hi Eddy
Where can I access this paper? Thanks
Stephen [HSP]
Look at the CVnet
Hi Stephen,
Look at the CVnet site.
Regards,
Eddy
Thanks, Eddie. Got it.
XY Psc is given as UG: in VSX. Is it proven to be a UGWZ? If so, do you have a refrence?
Stephen [HSP]
No Stephen it's not proven but it looks like it is a UGWZ. Look at :
http://www.konkoly.hu/cgi-bin/IBVS?5140
Cheers,
Eddy
One of the criteria used by Taichi Kato in his paper is:
"the presence of early superhumps (reflecting the 2:1 resonance) and long or multiple rebrightenings are the best distinguishing properties of WZ Sge-type dwarf novae."
I suspect the reason for not including this star is that such early superhaumps have not been detected (yet)
We must continue to observe (when weather permits!!!!!!)
Kind regards
Stephen [HSP]