Chemical pumping from formation and destruction processes significantly enhances CH+ ro-vibrational populations and emission lines in NGC 7027 beyond radiative and inelastic collisions alone.
(2017), based on the more accurate but expensive time- dependent wave-packet (TDWP) method, and a good agreement (within a factor of
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Chemistry and ro-vibrational excitation of CH$^+$ in the planetary nebula NGC 7027
Chemical pumping from formation and destruction processes significantly enhances CH+ ro-vibrational populations and emission lines in NGC 7027 beyond radiative and inelastic collisions alone.