Abstract
THE oxygen second negative band system is a result of the transition A2Πu − X2Πg. It is a system of red-degraded double-headed bands, extending from 1900 Å to 6500 Å, and the separation of the heads of each band is 200 cm−1. The bands were first observed by Johnson1 and further identifications have been made by other workers2–6. A list of band-head wavelengths, taken from refs. 1–5, has been published by Wallace7. The frequencies of the band heads are given by
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References
Johnson, R. C., Proc. Roy. Soc., 105, 683 (1924).
Ellsworth, V. M., and Hopfield, J. J., Phys. Rev., 29, 79 (1927).
Mulliken, R. S., and Stevens, D. S., Phys. Rev., 44, 720 (1933).
Lal, L., Phys. Rev., 73, 255 (1948).
Feast, M. W., Proc. Phys. Soc., A, 63, 557 (1950).
Byrne, J., Proc. Phys. Soc., A, 78, 1074 (1961).
Wallace, L., Astrophys. J. Suppl., 7, 165 (1962).
Linton, C., Ph.D., thesis, London (1966).
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LINTON, C. New Identifications in the Oxygen Second Negative System. Nature 212, 1358 (1966). https://doi.org/10.1038/2121358a0
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DOI: https://doi.org/10.1038/2121358a0