ABSTRACT
The fine and hyperfine structure of the (0, 0) band of the B2Sigma+u-X2Sigma+g system of 14N+2 has been measured using fast-ion-beam laser spectroscopy. Rotational transitions with 0 = N" = 35 were recorded with a linewidth of approximately 0.0064 cm-1 full-width-half-maximum, allowing complete resolution of all strong hyperfine components. The frequencies of the line centers for N" >/= 3, together with the complete rotational line profiles for N" < 5, were used to determine the spin-rotation constants and the Fermi and dipolar hyperfine constants for the B and X states. This is the first time the hyperfine constants for v" = 0 have been measured for gas-phase N+2. Copyright 1998 Academic Press.
ABSTRACT
We have observed for the first time the (4, 4), (4, 3), and (5, 4) bands of the B 2Sigma+-X 2Sigma+ system of SiO+ using laser-induced fluorescence spectroscopy on a fast SiO+ beam. These data contain avoided crossings between the X 2Sigma+ and A 2Pi states, as well as a few extra lines belonging to the (3, 2), (4, 2), and (5, 3) bands of the B 2Sigma+-A 2Pi system. They enlarge considerably a previously measured data set consisting of almost 1400 lines of the (0, 0), (1, 1), (2, 2), (3, 3), (1, 0), (2, 1), and (3, 2) bands of the B-X system and 66 lines of the (2, 0) Omega = (1/2) subband of the B 2Sigma+-A 2Pi system. The entire data set of 2378 assigned lines has been fit simultaneously to a model Hamiltonian in which many closely overlapped levels of the X and A states are handled by direct diagonalization. The newly observed avoided crossings between the X and A states allow the determination of many A-state parameters with increased precision, several for the first time, including the spin-orbit splitting. The analysis confirms our earlier reinterpretation of older photoelectron spectroscopy data and allows the accurate prediction of the frequencies of strong infrared transitions between the X and A states, which have astrophysical significance. Copyright 1998 Academic Press.