Emission coefficients for gaseous nebulae - Three-level atom approximations

Details Emission coefficients for gaseous nebulae - Three-level atom approximations Emission coefficients for gaseous nebulae - Three-level atom approximations

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.208..253m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 208, May 15, 1984, p. 253-259. Research supported by th

Astronomy and Astrophysics

Astronomy

75

Atomic Spectra, Emission Spectra, Interstellar Gas, Nebulae, Argon, Neon, Nitrogen, Oxygen Spectra, Sulfur

Scientific paper

The recent compilation of atomic data by Mendoza (1983) has been used to construct three-level atom formulae for the emission coefficients for forbidden N II, O I, O II, O III, Ne III, S II, S III, and Ar III as a function of temperature and density. Equations for determining forbidden O II and S II densities and forbidden N II and O III temperatures are presented also. The formulae generally predict emission coefficients and ratios to within 5 percent of the five-level atom calculations, so should be of considerable value for analyses of gaseous nebulae spectra.

Affiliated with

Also associated with

No associations

Rating

Emission coefficients for gaseous nebulae - Three-level atom approximations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Emission coefficients for gaseous nebulae - Three-level atom approximations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Emission coefficients for gaseous nebulae - Three-level atom approximations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1369507