ASASSN-21mh: SU UMa star
Superoutbursts in the ZTF data. Time-resolved
ZTF data on 2020 July 13 detected superhumps.
The superhump period was near 0.06 d.
ASASSN-17eg: refined period and about type
Using the ZTF data, I obtained a refined orbital
period of 0.07859690(5) d. The mean light curve
is unlike that of an short-period dwarf nova
or novalike, but is a smooth sinusoidal one
with a full amplitude of 0.26 mag.
The object looks like to me basically a reflection
variable. The 2019 outburst likely came from
an accretion disk formed by a small amount of
mass-transfer. The transverse velocity is twice
larger than that of OV Boo and ASASSN-…
[View More]17eg is
probably a population II binary.
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CSS J062450.1+503114: superhump period
Itoh-san and Josch Hambsch have reported observations.
Well-defined superhumps have been observed and the period
has been established to be 0.07768(2) d. The mean amplitude
is 0.19 mag.
WFI J161953.3+031909: genuine eclipsing Z Cam (+SU UMa?) star in the period gap
ZTF data indicate that this object is a genuine Z Cam
star. Long standstill in 2021 Feb.-Sep. There has been
no indication of the IW And-type phenomenon.
Long outbursts in 2019 may have been superoutbursts.
The supercycle(?) was 70-90 d with a long duty cycle.
This would be classified as UGZ+UGSU(ER):+E.
ASASSN-22cw: most likely new WZ Sge-type dwarf nova
Berto Monard has reported observations. Two cycles
of variations were recorded. The period was 0.0528(7) d
and a full amplitude of 0.08 mag. The profile is
doubly humped with the second one brighter and this
suggests that the variation early superhumps.
Note that the period may be shorter than 0.05332 d
in GW Lib. Further observations are needed to
confirm and then update the period.