The optical spectrum was detected first in the laboratory by and later in the tail of comet . We have previously reported the observation by difference freqnency spectrometer of the vibration-rotation infrared spectrum of in the region using an A.C. glow discharge through He, and (100:1:1). The observed lines were assigned to the vibration-rotation band of that molecular ion. The band was not observable unlike the case of isoelectronic radical for which the transitions were reported to be much stronger than the transitions. The ground state molecular constants of Lew have been improved by including ground state combination differences from our data in the fit. A Watson reduced asymmetric rotor Hamiltonian, including the spin rotation interaction was used. The Coriolis interaction between the and vibrations has been included in the Hamiltonian to determine the excited state molecular constants for the first time.
Description
H. Lew, I. Heiber, J. Chem. Phys., 58, 1246 (1972) 2 P. A. Wehinger, S. Wyckoff, G. H., Herbig. G. Herzberg, H. Lew, Ap. J. ,190, L43 (1974) Address of Dinelli, Crofton and Oka: Department of Chemistry and Department of Astronomy and Astrophysics, The University of Chicago, Chicago, Illinois 60637 Permanent address of Dinelli: Istituto di Spettroscopia Molecolare del C.N.R., Bologna, Italy