[vsnet-outburst 25871] Mis V1448 in outburst! (since Oct. 16)

Sun Oct 18 05:30:50 JST 2020

 Mis V1448 (UG)
https://www.aavso.org/vsx/index.php?view=detail.top&oid=2213772

The current outburst (the first recorded one since 2012 May-July)
was also and independently detected by
1) Patrick Wiggins on CCD images that were taken by him on
my request (in the course of our CV monitoring programme);
the images were measured by Daniel Bamberger
2) the Zwicky Transient Facility (ZTF)
as follows:
MisV1448 20201015.146 16.96CR (Patrick Wiggins, Daniel Bamberger, and Patrick Schmeer)
MisV1448 20201016.172 16.44CR (Patrick Wiggins, Daniel Bamberger, and Patrick Schmeer)
MisV1448 20201017.170 12.93CR (Patrick Wiggins, Daniel Bamberger, and Patrick Schmeer)
MisV1448 20201017.202 12.87zg (Zwicky Transient Facility Lasair (Masci+ 2019))

Zwicky Transient Facility (ZTF) light curve:
https://lasair.roe.ac.uk/object/ZTF18abvazxu/

Recent ASAS-SN Sky Patrol (Shappee et al. 2014ApJ...788...48S
and Kochanek et al. 2017PASP..129j4502K) light curve and data:
https://asas-sn.osu.edu/light_curves/83231edb-c4cb-4f84-b4c6-1b2c890a5e84
MisV1448 20201014.256 <17.41g ASN

Recent astrometry (RA and DE J2000.0, Gaia DR2 reference stars;
observer Patrick Wiggings, measurer Daniel Bamberger):
2020-10-15.146 UT, 19:59:19.41 +/- 0.17", +56:25:20.95 +/- 0.16"
2020-10-16.172 UT, 19:59:19.43 +/- 0.18", +56:25:20.85 +/- 0.16"
2020-10-17.170 UT, 19:59:19.44 +/- 0.15", +56:25:20.71 +/- 0.15"
These results *might* indicate that the outbursting object is
a close companion to the mag. 17 star. OTOH, the third postion
is closest to the Gaia DR2 position of the mag. 17 star.

The 2012 outburst began between April 10 and 2012 May 13
(MASTER-Amur observations; Denis Denisenko, vsnet-alert 14643).
By June 9 it had faded to mag. 15.1 CR (vsnet-alert 14661).
A rebrightening was observed on July 3 (vsnet-alert 14727, 14731).
MASTER light curve:
http://master.sai.msu.ru/static/OT/MisV1448-2012outburst.gif

Such long outbursts with rebrightening(s) are often observed
in WZ Sge-type dwarf novae. However, the reported period of
0.183 d (4.4 h) is above the period gap; if correct, it would
indicate an SS Cyg-type dwarf nova.

Time-resolved photometry, spectroscopy, and further precise
astrometry are encouraged.

Clear skies,
Patrick
-------
     Am Samstag, 17. Oktober 2020, 01:03:56 MESZ hat 'Eddy Muyllaert' muyllaert.eddy at telenet.be [baavss-alert] <baavss-alert at yahoogroups.com> Folgendes geschrieben:  

MISV1448           20201016.8472 13.2       OUTBURST!

Regards,

Eddy
  __._,_.___     Posted by: "Eddy Muyllaert" <muyllaert.eddy at telenet.be>     
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