Fluorescence efficiencies of the A-X and B-X systems of CO 2 + in comets
© The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences. 1999
Received: 6 May 1998
Accepted: 20 October 1998
Published: 6 June 2014
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.