Determination of the intrinsic Q(3)/5(1) line intensity ratio of molecular hydrogen

Details Determination of the intrinsic Q(3)/5(1) line intensity ratio of molecular hydrogen Determination of the intrinsic Q(3)/5(1) line intensity ratio of molecular hydrogen

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982stin...8229247g&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Atmospheric Attenuation, Emission Spectra, Hydrogen, Line Spectra, Molecular Clouds, Planetary Nebulae, Absorption Spectra, Astronomical Spectroscopy, Flux Density

Scientific paper

Observations of the H2 Nu = 1 yields O S(1) and Q(3) lines in the
planetary nebula NGC 7027 yield an intrinsic Q(3)/S(1) line intensity
ratio of 0.74 + or - 0.08. This value is consistent with the theoretical
ratio of the Einstein A coefficients of these transitions. The HI 20-5
line intensity in NGC 7027 is also reported and discussed.

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