Home Page Updated on November 1, 2017
MisV0372 = V5382 Sgr
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.
Taichi Kato pointed out that this object is within the positional error range of a X-ray source 1RXPJ180245-2942.3 at R.A. 18h02m45s.6, Decl. -29o42'20" (2000.0).
Taichi Kato and John Greaves pointed out the possible identification with an X-ray star 1RXP J180245-2942.3. But it is revealed to be a normal Mira type variable based on the OGLE-II data.
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