Discovery of a Probable Nova in M31
ATel #7603; K. Hornoch (Astronomical Institute, Ondrejov, Czech Republic), H. Kucakova, K. Honkova and J. Vrastil (Astronomical Institute, Charles U., Prague, Czech Republic)
on 7 Jun 2015; 21:38 UT
Credential Certification: Martin Henze (martin.henze@sciops.esa.int)
Subjects: Optical, Nova, Transient
Referred to by ATel #: 7789
We report the discovery of rather faint, slowly rising probable nova in M31 on a co-added
1320-s R-band CCD frame taken on 2015 May 31.030 UT with the 0.65-m telescope at Ondrejov.
The object is well visible also on a few pre-discovery images, but is not present on many
archival images taken with various telescopes during last several years. Also, the object
is not visible on R-band images of the Survey of Local Group Galaxies Currently Forming
Stars: I. UBVRI Photometry of Stars in M31 and M33 by Massey et al. (2006, AJ, 131, 2478)
down to R ~ 21.5 mag.
The object designated PNV J00423445+4116443 is located at R.A. = 0h42m34s.45,
Decl. = +41o16'44".3 (equinox 2000.0), which is 111.3" west and 35.8" north
of the center of M31 (see link to image taken on Jun. 3.047 UT below).
The following R-band magnitudes (unless otherwise noted) were obtained using
the 0.65-m telescope at Ondrejov:
2015 Apr. 25.101 UT, [20.2; May 11.057, 18.8 ± 0.3; 12.072, 18.8 ± 0.3;
16.063, 19.2 ± 0.35; 31.030, 18.7 ± 0.25; Jun. 3.047, 18.3 ± 0.2;
5.007, 18.3 ± 0.2; 5.020, I = 17.7 ± 0.3; 6.024, 18.1 ± 0.15;
6.985, 18.2 ± 0.2.
A search for known variable sources close to the position of the PNV J00423445+4116443
did not reveal any known variable object located closer than 2.8" from the position
of PNV J00423445+4116443. The closest known variable object is M31N 2008-03b
discovered by K. Hornoch on 2008 Mar. 7.756 UT. A direct comparison of the best images
available for M31N 2008-03b and PNV J00423445+4116443 shows that they are
undoubtedly two distinct objects.
The observed (R-I) ~ 0.6 mag is consistent with a nova around maximum brightness,
but would be atypical for a red LPV. Nevertheless, spectroscopic classification
is strongly encouraged to firmly establish the nature of the object.
Image of the PNV J00423445+4116443