The system Bm Ori. V. Improved photometric elements |
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| Authors: | É. A. Vitrichenko |
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| Affiliation: | (1) Institute for Space Studies, Russian Academy of Sciences, Moscow, Russia |
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| Abstract: | The times of individual minima taken from the literature are used to plot the dependence of O-C on revolution number for the eclipsing star BM Ori. A least squares fit of this plot yields the following photometric elements: Min I=JD2440265.331(5)+6.470524(3)·E. __________ Translated from Astrofizika, Vol. 51, No. 3, pp. 501–503 (August 2008). |
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| Keywords: | stars eclipsing binary Orion Trapezium BM Ori |
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