AN EMISSION SYSTEM OF THE IO MOLECULE
dc.creator | Durie, R. A. | en_US |
dc.creator | Legay, F. | en_US |
dc.creator | Ramsay, D. A. | en_US |
dc.date.accessioned | 2006-06-15T12:54:11Z | |
dc.date.available | 2006-06-15T12:54:11Z | |
dc.date.issued | 1959 | en_US |
dc.identifier | 1959-B-1 | en_US |
dc.identifier.uri | http://hdl.handle.net/1811/7804 | |
dc.description | $^{1}$ Coleman, E.H., Gaydon, A. G. and Vaidya, W. M. Nature 162 , 108 (1948). | en_US |
dc.description | Author Institution: Division of Pure Physics, National Research Council, Ottawa | en_US |
dc.description.abstract | A band system of the IO molecule, first observed by Coleman, Gaydon and $Vaidya^{1}$ in emission from an oxyhydrogen flame to which methyl iodide was added, has been photographed under high resolution using a 21 ft. concave grating spectrograph. Approximately forty bands have been observed in the region 4000 to 7000 {\AA}. The rotational structure of the bands indicates that the transition is of the type $^{2}\Pi {}^{2}\Pi$. The analysis of the bands and the molecular constants of IO will be discussed. | en_US |
dc.format.extent | 53235 bytes | |
dc.format.mimetype | image/jpeg | |
dc.language.iso | English | en_US |
dc.publisher | Ohio State University | en_US |
dc.title | AN EMISSION SYSTEM OF THE IO MOLECULE | en_US |
dc.type | article | en_US |
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