Swift J1727.8-1613: black-hole binary and V404 Cyg-like object ?
Swift and MAXI detected an outburst in Swift J1727.8-1613.
This is a candidate for a black-hole binary and possibly similar to
V404 Cyg, a unique object known as a source of rapid variability.
A few seconds variability was already found in X-rays.
The most violent variability would be ~2 mag in several tens of min.
This is very bright. Currently, ~13 mag.
The position is (RA)17:27:46 (DEC)-16:12:53 reported by Swift.
Follow-up …
[View More]observations are strongly encouraged.
https://www.astronomerstelegram.org/?read=16205https://www.astronomerstelegram.org/?read=16208
- Mariko Kimura at Kanazawa Univ. in Japan
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MASTER OT J183342.09+654019.1 superoutburst
Superhumps of this object were observed in 2021 Apr.,
but not so well.
YYYYMMDD(UT) mag observer
20230803.2927 17.662g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014))
20230805.3107 17.534g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014))
20230814.4402 17.555g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014))
20230822.4005 15.150g (ASAS-SN Sky Patrol Photom. DB (Hart+2023; Shappee+2014))
(forwarded …
[View More]message)
===
From: <andrew_simon(a)univ.kiev.ua>
Date: Fri, 25 Aug 2023 22:43:27 +0300
Dear Dr. Taichi Kato,
According to my observations in the Lisnyky observational station during
the last two nights it looks like the object Gaia19cuu now in
superoutburst. From the observations superhumps can be easily detected on
the images attached to this letter.
Data from the Gaia shows previous outbursts with the amplitude of 4-5
magnitudes (https://gsaweb.ast.cam.ac.uk/alerts/alert/Gaia19cuu/)
Also data from Gaia Followup for 7 Jul 2019 submitted by Liam Hardy shows
superhumps, due to these data I started to follow this object. (
https://gsaweb.ast.cam.ac.uk/alerts/alert/Gaia19cuu/followup)
ZTF also detected multiple outbursts in the light curve as well as current
outburst. https://lasair-ztf.lsst.ac.uk/objects/ZTF18aatluwz/
After analysing the data I found 0.068d period for 2023-08-23 and 0.077d
period for 2023-08-24. But due to the relatively short duration of
observations these determinations can be not precise. Obtained data
relatively to the comp.star I also attached to this letter.
This night it is cloudy in Kyiv so I have no possibility to
continue observations. But I hope that the object will appear to be
interesting for observations over the world.
Best regards,
Andrew Simon.
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> The UGSU-type dwarf nova FZ Cet is in outburst according to NMW survey
> photometry (135mm f/2.0 lens + unfiltered STL-11000 CCD):
Please pay attention not to post a new message as a reply
to an old, unrelated message.
See how your posting looks like:
http://ooruri.kusastro.kyoto-u.ac.jp/mailman3/hyperkitty/list/vsnet-alert@o…
Blazar 1ES 1959+650 in optical high state
object date (UTC) mag comment
--------------------------------------------------
1959+650 20230717.874 14.17V active (1)
1959+650 20230805.109 14.06V active (1)
1959+650 20230812.…
[View More]952 13.99V active (1)
--------------------------------------------------
The optical high state corresponds well with strong X-ray
activity detected by Swift-XRT (see Atel #16186).
--------------------------------------------------
(1) 30cm-Refl. + CCD + V-Johnson (remote)
Stefan Karge (SKA)
http://quasar.square7.ch/fqm/1959+650.html
_______________________________________________
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