[vsnet-alert 2774] Brightening of HadV14 = Wra 1292

[Taichi Kato <tkato>]

Brightening of HadV14 = Wra 1292

   As reported in vsnet-obs 19699, Katsumi Haseda (Aichi, Japan) discovered
the brightening of a new variable star (HadV14), which has been subsequently
identified with a cataloged emission-line object Wra 1292.  The photometric
record indicates the object has been in bright state at least for these
three months.  The object is neither red in the USNO color, nor included
in the IRAS catalogues.  It may be a unique brightening of a peculiar object,
such as a symbiotic variable.  Spectroscopic determination of the object type
is therefore encouraged, with continued photometric monitoring.

HadV14
= GSC7826.572 151024.39 -405428.3 (2000.0) 12.82 0
= USNO0450.19726095 151024.384 -405428.44 (2000.0) 13.7 12.5
= 151024.4 -405427 (2000.0) WRA1292

object         YYMMDD(UT)   mag  code
HadV14         960305.797  123p  Had.VSOLJ
HadV14         960325.745  <146p  Had.VSOLJ
HadV14         970112.850  <138p  Had.VSOLJ
HadV14         970305.800  <148p  Had.VSOLJ
HadV14         980205.831  133p  Had.VSOLJ
HadV14         980226.797  123p  Had.VSOLJ
HadV14         990121.843  121p  Had.VSOLJ
HadV14         990221.819  126p  Had.VSOLJ
HadV14         990313.771  125p  Had.VSOLJ

VSNET Home Page

Return to Daisaku Nogami

---

vsnet-adm@kusastro.kyoto-u.ac.jp