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Dear colleagues, Photographic observations were reported from Kesao Takamizawa and Katsumi Haseda in [vsnet-newvar 1194] and [vsnet-newvar 1196] on Nov. 7, 2001. Takamizawa commented that "The star may be a Mira-type variable with a range of 11.4-<14.3p, and a period about 340days". I analyzed their observations with MISAO's observations. Here is the summary: http://vsnet.aerith.net/misao/variable/special-note.html#MisV0200 Here is the light curve: http://vsnet.aerith.net/misao/report/variable/MisV0200.gif MisV0200 is a Mira type variable. Speaking of the period, period of about 350 days seems to fit the observations better than that of about 340 days. One of the peak was around 2452205 (JD). We reported MisV0200 with an unfiltered CCD brightness range of 11.5 - 12.5 mag on Aug. 22, 1999. But observations by the MISAO Project were at faint phases when photographic brightness is fainter than 13.5 mag, so the unfiltered CCD peak brightness seems to be much brighter than 11 mag. Best regards, -- Seiichi Yoshida comet@aerith.net http://vsnet.aerith.net/
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
