Abstract
Fluorescence models of the A-X and B-X band systems of CO 2 + have been constructed using molecular parameters available in literature. The models have been compared with the spectra of comets Austin (1989c1) and P/Giacobini-Zinner. From the best fit, the fluorescence efficiencies of the A-X and B-X band systems have been derived.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Paper version not known
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
