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2O will be patchy within our beam. There is evidence that the disk of α Ori is not uniform in brightness [see, for example, V. A. Klückers, M. G. Edmunds, R. H. Morris, N. Wooder, Mon. Not. R. Astron. Soc. 284, 711 (1997)]. If the water exists in localized areas, a model using a filling factor for water, rather than a uniform chromospheric layer, would be more appropriate. Observationally, a nonuniform distribution of water might make it possible to detect changes in the spectra as the star rotates.
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6844243216
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note
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The authors thank P. Bernath, K. Hinkle, and L. Wallace for supplying preprints; D. Deming, D. Reuter, and G. McCabe for discussions; R. Boyle, K. McFarland, and E. Zamkoff for assisting during the observations; G. Bjoraker for supplying line strengths; and the staff of the National Solar Observatory. The National Solar Observatory is a division of the National Optical Astronomy Observatories, which is operated by the Association of Universities for Research in Astronomy, under contract with the National Science Foundation. Celeste was manufactured by IR Systems, and its electronics were manufactured by Wallace Instruments. The BIB detector array was manufactured by Boeing Research and Technology Center.
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