Home Page Updated on April 20, 2018
MisV0255 = V1679 Aql
= IRAS 18592+1455 R.A.=19 01 31.88 Decl.=+15 00 19.1 (19 x 4", p.a. =78) flux(12)=37.65 flux(25)=25.15 flux(60)=4.35 flux(100)=<4.12 99% variable
It was detected by the PIXY system as one of the candidates of new variable stars from images taken by Ken-ichi Kadota, Ageo City, Saitama, Japan, then confirmed by Seiichi Yoshida.
Research and Publication
Light curve by the Northern Sky Variability Survey (NSVS) created using SkyDOT.
SkyDOT is operated by the University of California for the National Nuclear Security Administration of the US Department of Energy.
Observations by MISAO Project