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.
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
