Home Page Updated on March 15, 2018
MisV0074 = V1259 Sco
= IRAS 17531-3110 R.A.=17 56 23.75 Decl.=-31 10 49.8 (26 x 5", p.a. =92) flux(12)=2.04 flux(25)=1.45 flux(60)=<7.29 flux(100)=<89.21 98% 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 Analysis of MisV Stars Identified with Candidate Variable Stars from OGLE-II Bulge Data
Yoshida, S.; Greaves, J.
Observations by MISAO Project