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The star IRAS14436-0703 is found to be a Mira star with a period of 297 days, by inspecting Stardial images (http://vsnet.astro.uiuc.edu/stardial/). The amplitude in unfiltered light is around 3 magnitudes or more, and the maximum and minimum seem to vary by about a magnitude. Epoch of maximum light JD 2452045, M-m = 0.4. From USNO B1.0, B-R is somewhat larger than 3.0. Using VizieR, I could come up with the following identifications: USNO-A2.0 0825-08448548 GSC 2.2 S23103201703 USNO-B1.0 0827-0352688 Image reduction has been done by using the XVista programs written by Michael Richmond, who is gratefully acknowledged. Patrick __________________________________________________ Do you Yahoo!? Yahoo! Platinum - Watch CBS' NCAA March Madness, live on your desktop! http://platinum.yahoo.com
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
