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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
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.
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- Copyright © Cambridge University Press 1989