CH Her superhump period
Tamas Tordai has reported second-night observations.
The superhump period is established to be 0.07398(3) d.
The amplitude is 0.15 mag.
Gaia DR3 2893005857946801152 = ASASSN-23dr: superhump period
Berto Monard and Josch Hambsch have reported further
observations. Thanks to Monard's high-cadence data,
it has become apparent that ordinary superhumps started
to appear on May 19. Due the the gap in the observation,
I analyzed the data since May 22 and obtained a superhump
period of 0.0580(1) d (amplitude 0.10 mag and the existence
of superhumps is unambiguous). I could not detect early
superhumps corresponding to this period,…
[View More] but as I already
reported, this object appears to be a WZ Sge star.
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