A NEW BAND SYSTEM IN THE NEAR-ULTRAVIOLET SPECTRUM OF MAGNESIUM OXIDE

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1964

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Ohio State University

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The apparent complexity and the previously observed irregular isotope shift in the near-ultraviolet band spectrum of magnesium oxide1 gave ground for speculation that the bands may be caused by a polyatomic emitter or overlapping triplet transitions of MgO. The are spectrum of MgO in the 3750−3900\AA region has been reinvestigated. Rotational lines of the MgO16 and MgO18 spectra have been measured from plates taken with a 21-ft. concavegrating spectrograph in the second order. It was found that the C1ΣA1Π system reported earlier2 extends to about 3795\AA. The bands from 3795\AA to the longer wave lengths are members of a D1ΔA1Π system and from a zero sequence. The Λdoubling is clearly observed in the R∗,∗, band head region. The preliminary values of the rotational constants and vibrational frequency for the new D1Δ state are: Bo=0.499,B1=0.494,Do=D1=1.3×10−6 and ωe=632cm−1.

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1 D. Pesic, Proc. Phys. Soc. London A 76, 844 (1960). 2 L. Brewer, S. Trajmar and R. Berg, The Astrophysical Journal 135, 455 (1962).


Author Institution: California Institute of Technology, Jet Propulsion Laboratory, 4800 Oak Grove Dr; \dag Present address: Department of Chemistry, Indiana University, Bloomington, Indiana

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