Relative Intensities of Hydrogen Recombination Lines in Gaseous Nebulae

Details Relative Intensities of Hydrogen Recombination Lines in Gaseous Nebulae Relative Intensities of Hydrogen Recombination Lines in Gaseous Nebulae

Sep 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967natur.215.1365d&link_type=abstract

Nature, Volume 215, Issue 5108, pp. 1365 (1967).

Physics

Scientific paper

RECENTLY, Gardner and McGee1 have published measurements on the 126α, 159β and 158β recombination lines of hydrogen in two galactic nebulae. These lines have frequencies differing by less than 2 per cent and are therefore observed with the same beamwidth. Their results are summarized in Table 1. TL is the measured peak line temperature above the continuum. (TLβ/TLα)E is the predicted ratio of temperatures assuming thermodynamic equilibrium and equal line widths.

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