ASASSN-22gb: stage A superhumps
Berto Monard and Josch Hambsch have reported further
observations. The amplitudes of superhumps have been
growing and the maxima were expressed by 0.05442(5) d
(stage A superhumps). The long duration of stage A suggests
a relatively small q.
ASASSN-22gm: eclipsing AM CVn star
Berto Monard has reported observations. I obtained
the following ephemeris (single night):
BJD(Min) = 2459705.53602(7) + 0.02890(3) E
Eclipse depth 0.26 mag. No superhumps were detected.
The orbital profile is somewhat strange in that it
showed two maxima in one orbital cycle.
They might be (super)hump-like variations with a period
of the orbital period. The object is most likely
an eclipsing AM CVn star with infrequent outbursts.
Further …
[View More]observations are needed to see whether this
was a precursor or an isolated normal outburst.
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