Home Page Updated on December 16, 2020
MisV0531ProfileMisV0531
Digitized Sky Survey GIF image (15 x 15 arcmin) Discovery InformationIt 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. Special NotesStefan Huemmerich and Klaus Bernhard revealed that it is a Mira type variable with a period of 356 days, brightness range of 11.8-15.9 mag(Rc), using the MACHO project data. Light Curve12.5 +--------------------------------------------------------+ | * | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | * | | | | | | * | 14.7 +--------------------------------------------------------+ 2451269 2451453 1999 Mar. 31 1999 Oct. 1 Observations by MISAO Project
|