Abstract
Abstract Emission resulting from collisions of 100–1000 eV He· and He2· ions with CH3HgBr molecules has been characterized in the 244–580 nm region. Emission bands due to HgBr (B-X), CH(A-X), and CH(B-X) transitions were observed besides atomic mercury lines. Emission cross-sections as a function of energy of helium ions for the strongest band of HgBr radical at 502 nm corresponding to the transition (v' = 0 − v′ = 22) were determined.
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