Key points are not available for this paper at this time.
Hydrogenic emission and recombination coefficients are presented which cover extremes of both wavelength (912 A to 20 microns) and temperature (electron temperature of 500-2,000,000 K). These tables should facilitate interpretation of both satellite and ground-based observations of exotic gaseous nebulae.
G. J. Ferland (Wed,) studied this question.