Confirmation of PNV J13544700-5909080 and Identification of a Probable Progenitor
ATel #5621; K. Hornoch (Astronomical Institute, Ondrejov, Czech Republic)
on 3 Dec 2013; 11:17 UT
Credential Certification: Martin Henze (mhenze@mpe.mpg.de)
Subjects: Optical, Nova, Transient
Referred to by ATel #: 5628
Information about the discovery of a bright possible nova in Centaurus
by J. Seach, Chatsworth Island, NSW Australia, designated PNV J13544700-5909080
was posted here.
I confirm the presence of the bright object (R ~ 5 mag) on 0.3-s R-band images obtained
using the Danish 1.54-m telescope at La Silla on 2013 Dec. 3.361 UT. The object
is located at R.A. = 13h54m45s.34, Decl. = -59o09'04".2 (equinox 2000.0).
The object is very probably identical with a ~ 15 mag star
USNO-B1.0 0308-0442031 = 2MASS 13544534-5909040 = UCAC4 155-128029,
which I identify as a probable progenitor of the possible nova. If the identification
is correct, the estimated amplitude of the outburst is ~ 10 mag, which is consistent
with the outburst of a classical nova.
Comparison of a combined R-band image from the Danish 1.54-m telescope (left) with DSS-2
red image (right) is posted here
Based on data collected with the Danish 1.54-m telescope at the ESO La Silla
Observatory.
