Abstract
The 115-750-nm radiation produced in collisions of 1.5-25-keV H+ and H with O2 has been studied in an atomic-beam experiment under thin-target conditions. For both ion and neutral impact, the (bΣg4aΠu4) first-negative (1N) and (AΠu2XΣg+2) second-negative (2N) band systems of O2+ are the most intense spectral features. Also observed are several emissions from excited states of O and O+. Relative cross sections for individual bands of the O2+ 1N system, obtained by deconvolution of overlapped features in several vibrational sequences, were used to show that the vibrational population P(v) for O2+ bΣg4 formed in both H+ and H impact is in good agreement with the predictions of a simple Franck-Condon mechanism over the 2-25-keV energy range. Total cross sections for formation of O2+ bΣg4 in H+ and H impact, determined from the latter results by normalization to previous proton-impact data, are in good agreement with values calculated via application of the semiempirical procedure developed recently by Edgar et al. For both projectiles the semiempirical approach gives a good prediction of the energy dependence and an adequate prediction of the magnitude of the cross sections for formation of O2+ AΠu2 determined by integration of measured 2N band intensities.