Abstract
In stellar atmospheres and regions of the interstellar medium with electron densities above 104 cm-3, three-body recombination into high levels of the hydrogen atom with principal quantum numbers k >> 1 can play a more important role than radiative recombination into lower states.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
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
