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HgBr (B–X) formation due to collisions involving O+/ and HgBr2 at kinetic energies (lab.) above 100 eV

Published online by Cambridge University Press:  09 March 2009

Mohammad F. Mahmood
Mohammad F. Mahmood
Affiliation:
Department of Electrical Engineering Howard University, Washington, D. C. 20059 U.S.A.
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Abstract

The emission spectra of HgBr (B–X) band system and atomic mercury lines have been observed during collisions involving O+/ and HgBr2 in the kinetic energy (lab.) range of 100–1000 eV.

Type
Research Article
Information
Laser and Particle Beams , Volume 7 , Issue 4 , November 1989 , pp. 829 - 833
Copyright
Copyright © Cambridge University Press 1989

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