Affiliation
Association Francaise des Observateurs d'Etoiles Variables (AFOEV)
Sun, 04/29/2018 - 16:10
V392 Persei (UG)
https://www.aavso.org/vsx/index.php?view=detail.top&oid=25916
"2018 04 29.4740 UT
Yuji Nakamura, Kameyama, Mie, Japan, reports his discovery of this TCP (mag 6.2) in Per on a CCD frame taken on 2018 Apr 29.4740 UT (limiting mag 12.5) using a 135mm f4.0 lens. The object was not shown on a frame taken on 2018 Apr 21.4627 UT (limiting mag 12.5). There is a UG type variable star V392 Per at this position."
http://www.cbat.eps.harvard.edu/unconf/followups/J04432130+4721280.html
Confirmation, spectroscopy, multiband photometry, and precise astrometry are very urgently required.
Clear skies,
Patrick
I don't know about rebrightening, but for my eye V392 Per has been holding rather steady for the past 6 nights. Tonight I estimated 8.6 mag.
Wasn't able to view yesterday, but seemed to plummet since two days ago, from 8.6 to 9.3. Maybe I did witness a rebrightening then.
Hi all,
V392 Per
06/05/2018 21:16 UT, "Doble Visual BINOCULAR": monocular 20*45: 8.8m (limit=+9.0m) + Refractor 60/600, 30*: 9.03m (limit=+9.3m); z=~80o;
07/05/2018 21:56 UT, "Double Visual BINOCULAR": monocular 20*45: 8.90m (limit=+9.0m) + Refractor 60/600, 30*: 8.78m (limit=+9.15m); z=~83o, MINSK, BELARUS.
V 392 Per 07.05.2018, 16.13UT/8,8, 9,0/ lim 9,3/z 75/ZT 10х30, Tatiana Donchenko, Tashkent, Uzbekistan.
10/05/2018 21:26 UT, "Double Visual BINOCULAR": monocular 20*45: No Star (limit=+8.9m) + Refractor 60/600, 30*: 9.4-9.5m (limit=+9.65m); z=~83o, Minsk, BELARUS.
the End /
Ivan S. Bryukhanov (BISA), Minsk, Belarus.