TCP J01535830+5937545: likely superoutburst of an SU UMa star
Type from ZTF data. Apparent superoutburst in 2019 Nov.
YYYYMMDD(UT) mag observer
20211010.6888 170:C (Masayuki Moriyama)
20211011.8173 163:C (Masayuki Moriyama)
Re: PNV J00444033+4113068: updated period of early superhumps
> Tamas Tordai and Tonny Vanmunster have reported new
> observations.
Sano-san also reported observations. The result
is unchanged.
PNV J00444033+4113068: updated period of early superhumps
Tamas Tordai and Tonny Vanmunster have reported new
observations. The best period using these observations
is 0.05543(2) d. The double wave profile is very
apparent. The deeper minima appear to be partially
caused by eclipses. These eclipses will become more
apparent when ordinary superhumps appear.
ASASSN-14cc (AM CVn star)
https://www.aavso.org/vsx/index.php?view=detail.top&oid=398940
Apparently not much activity in recent months: after a normal outburst on
2021 May 23, the only recorded brightening was a double outburst on
August 4-10 and 13-18, according to ASAS-SN Sky Patrol (Shappee et al.
…
[View More]2014ApJ...788...48S and Kochanek et al. 2017PASP..129j4502K) data.
https://asas-sn.osu.edu/sky-patrol/coordinate/d031a323-285e-44df-9854-81a0e…
Regards,
Patrick
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Taichi Kato wrote on Wednesday, 28 January 2015, 07:40:45 UTC:
ASASSN-14cc
Let's continue observations in the next season, too.
http://arxiv.org/abs/1501.06659
Title: ASASSN-14cc: Likely Helium Analog of RZ Leonis Minoris
Authors: Taichi Kato (Kyoto U), Franz-Josef Hambsch (GEOS, BAV, Vereniging Voor
Sterrenkunde), Berto Monard (Center for Backyard Astronomy Kleinkaroo)
Categories: astro-ph.SR
Comments: 5 pages, 5 figures, accepted for publication in PASJ (Letters)
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
\\
We identified that ASASSN-14cc is a very active dwarf nova spending
approximately 60% of the time in outburst. Our long-term photometry revealed
that the object shows long outbursts recurring with a period of 21-33 d and
very brief short outbursts lasting less than 1 d. The maximum decline rate
exceeds 2.8 mag/d. The duration of long outbursts is 9-18 d, comprising 50-60%
of the recurrence time of long outbursts. We detected 0.01560-0.01562 d (22.5
min) modulations during long outbursts, which we identified to be superhumps.
These features indicate that ASASSN-14cc has outburst parameters very similar
to the extreme dwarf nova RZ LMi but with a much shorter superhump period. All
the observations can be naturally understood considering that this object is a
helium analog (AM CVn-type object) of RZ LMi. The highest outburst activity
among AM CVn-type objects can be understood as the high-mass transfer rate
expected for the orbital period giving a condition close to the stability limit
of the accretion disk. In contrast to RZ LMi, this object shows little evidence
for premature quenching of the superoutburst, which has been proposed to
explain the unusual outburst parameters in RZ LMi.
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PNV J00444033+4113068: new WZ Sge-type dwarf nova
Tamas Tordai has reported observations. The object
showed large-amplitude (0.7 mag!) early superhumps
with a period of 0.0553(4) d.
This object must have a high inclination and
further observations are very encouraged.
LL Andromedae (UGWZ)
https://www.aavso.org/vsx/index.php?view=detail.top&oid=260
The rapid fading was already reported by me on Sept. 9 (vsnet-alert 26311).
It started around 2021 September 9.1 UT according to AAVSO data:
https://app.aavso.org/webobs/results/?star=000-BBB-961
Time-resolved photometry or at least daily snapshots …
[View More]are still encouraged.
Clear skies,
Patrick
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Filipp Romanov wrote on Monday, 11 October 2021 at 15:58:48 UTC:
Based on my observations (remotely from Burke-Gaffney Observatory,
Canada), rapid fading of LL And started after 2021-10-08:
2021 10 05.28754 14.76 V
2021 10 06.31925 14.84 V
2021 10 07.09830 14.94 V
2021 10 08.25946 15.06 V
2021 10 09.14966 15.50 V
I reported these observations and my other multicolour photometric
observations in the [vsnet-obs 94323].
With best regards,
Filipp Romanov (Russia).
------------
Taichi Kato wrote on Sunday, 10 October 2021 at 23:54:33 UTC:
LL And rapid fading
Itoh-san's most recent observation on Sep. 10
indicated that the object faded to 17th mag.
Please keep an eye on this object to look for
possible rebrightening(s).
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