Integrated fluxes for emission lines in the ultraviolet spectra of several planetaries

Details Integrated fluxes for emission lines in the ultraviolet spectra of several planetaries Integrated fluxes for emission lines in the ultraviolet spectra of several planetaries

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981stin...8213022c&link_type=abstract

Final Report, 15 Apr. 1980 - 30 Jun. 1981 Ohio State Univ., Cleveland. Dept. of Astronomy.

Astronomy and Astrophysics

Astronomy

Emission Spectra, Iue, Planetary Nebulae, Radiant Flux Density, Ultraviolet Astronomy, Ultraviolet Spectra, Calibrating, High Resolution, Interpolation, Ion Concentration, Ions, Plasma Density, Plasma Temperature

Scientific paper

The IUE satellite observatory was used to obtain absolutely-calibrated emission line fluxes for diagnostic lines of multiply-ionized C, N, O, Si, Ne, and Ar which occur in the ultraviolet spectral region of planetary nebulae. These data, when combined with data from the blue, visual, and near infrared, provide improved estimates of ionic concentrations, plasma temperatures and densities, and elemental abundances.

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