ASASSN-19wz possible superoutburst
Past ZTF data suggest an SU UMa star (possible superoutburst
in 2020 Nov.).
YYYYMMDD(UT) mag observer
20210901.2558 15.276zg (Zwicky Transient Facility Lasair (Masci+ 2019))
The AM CVn-type object NSV 1440 is in bright outburst.
NSV 1440 210830.519 129
--
Rod Stubbings
Tetoora Road Observatory
Victoria, Australia
Telescope: "Infinity" 22" f/3.8
stubbo(a)dcsi.net.au
http://rodstubbingsobservatory.wordpress.com/
ASASSN-V J205543.90+240033.5: combination of three periods
Josch Hambsch and Tonny Vanmunster have reported
observations.
See
https://arxiv.org/abs/2108.09060http://vsolj.cetus-net.org/vsoljno80.pdf
"ASASSN-V J205543.90+240033.5: another white dwarf pulsar?"
Their observations indicate that the global
variation is a combination of the longer period 10.803 d
and a shorter period 0.203424(1) d (determined from
the ZTF data). These variations create the dispersion
in figure 2 of the above paper.
Their data also confirmed the short period of
0.0067876(7) d (amplitude 0.07 mag).
This must be a very interesting CV-like object
and further observations (including spectroscopy)
are requested.
ASASSN-21qg: new SU UMa-type dwarf nova
Berto Monard and Josch Hambsch have reported observations.
This object shows superhumps with a period of 0.05539(5) d
since Aug. 26.