[vsnet-outburst 22121] Re: TCP J04432130+4721280 = V392 Per nova eruption (6.2 mag)?

Mon Apr 30 04:30:32 JST 2018

V392 Persei  (UG+N:)

CBAT "Transient Object Followup Reports" link:
http://www.cbat.eps.harvard.edu/unconf/followups/J04432130+4721280.html

The ASAS-SN Sky Patrol (Shappee et al. 2014ApJ...788...48S and Kochanek
et al. 2017PASP..129j4502K) recorded a dwarf nova outburst with a very
slow (GK Per-like) rise in 2016 February/March:
https://asas-sn.osu.edu/light_curves/adf2ab4d-f15c-496d-8493-5f747475cfeb

The very slow rise to outburst maximum indicates a long orbital period.

That 2016 February-April outburst was visually detected by Carey
Chiselbrook at mv= 14.2 on 2016 Feb. 28.04722 UT. The final AAVSO
observation before solar conjunction was made by Steve Johnston on
2016 Apr. 19.86573 UT (V= 14.341):
https://www.aavso.org/apps/webobs/results/?star=V392+Per&page=8

Btw, V392 Persei is located 6 degrees WNW of alpha Aurigae (Capella).

Regards,
Patrick
-------------------
Original message (vsnet-alert 22120/vsnet-outburst 22119):

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.