ASASSN-23af rebrightening
Josch Hambsch has reported that this object brightened
on Feb. 11 and is at 15.5. This behavior suggests a long
rebrightening of a WZ Sge star.
CRTS J103317.3+072119 bright outburst
Known SU UMa star, but single-night observation was available
in the past.
YYYYMMDD(UT) mag observer
20230120.6737 <157c (Yutaka Maeda)
20230121.6604 <157c (Yutaka Maeda)
20230130.6625 <157c (Yutaka Maeda)
20230204.6566 <152c (Yutaka Maeda)
20230210.7456 139cG (Yutaka Maeda)
ASASSN-15cm: SU UMa star with Porb=0.2085 d
Using ZTF (Masci et al., 2019) and ATLAS forced photometry
(Tonry et al. 2018; Shingles et al. 2021) data, I found
that this object showed a superoutburst in 2019 Aug.
Like BO Cet with the same set of data (arXiv:2302.02593 =
VSOLJ Variable Star Bulletin No. 106), I obtained a period
of 0.2196(1) d, 5.3% longer than the orbital period.
This corresponds to q about 0.22 (arXiv:2201.02945 =
VSOLJ Variable Star Bulletin No. 89).
The core of the …
[View More]secondary of this object appears to be
evolved (Thorstensen et al. 2016 AJ 152, 226) and
this probably enabled a relatively small q.
Another apparent superoutburst was also recorded in 2022 Jan.
and future direct detection of superhumps are wanted.
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Re: ASASSN-15cc bright outburst continues
> Time-resolved photometry is encouraged.
Itoh-san just reported observations on two nights.
No superhumps were present. SS Cyg star or superhumps
may appear?
PNV J06245297+0208207 brightened again
According to observations by Itoh-san and Tamas Tordai,
The object brightened to 13.5 mag on Feb. 10
(apparently oscillating with a time scale of about 1 d).
The brightening part on Feb. 9 was recorded by Crimean
Astrophys. Obs. team.
ASASSN-V J003612.92-464406.4: polar
Using ATLAS forced photometry (Tonry et al. 2018;
Shingles et al. 2021). Porb=0.0918846(1) d.
1.4-mag orbital variation. High and low states.