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MisV0547ProfileMisV0547
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 291.8 days, brightness range of 11.3-15.8 mag(Rc), using the MACHO project data. Light Curve12.2 +--------------------------------------------------------+ | * | | * | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | v | | | | v | | v | 14.7 +--------------------------------------------------------+ 2451269 2451453 1999 Mar. 31 1999 Oct. 1 Observations by MISAO Project
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