Electron density diagnostics for gaseous nebulae involving the O IV intercombination lines near 1400 A

Details Electron density diagnostics for gaseous nebulae involving the O IV intercombination lines near 1400 A Electron density diagnostics for gaseous nebulae involving the O IV intercombination lines near 1400 A

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apjs...88..169k&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 88, no. 1, p. 169-172.

Astronomy and Astrophysics

Astrophysics

12

Electron Density Profiles, Emission Spectra, Far Ultraviolet Radiation, Nebulae, Oxygen Spectra, Ultraviolet Spectra, Collisional Plasmas, Electron Energy, Electron States, High Resolution, Line Spectra, Optical Thickness, Protons, Temperature Dependence

Scientific paper

The Bloom and Pradhan (1992) results on the excitation rates for
transitions in O IV matrix are used to derive emission-line ratios near
1400 A, applicable to gaseous nebulae. The results are compared with the
values measured from high-resolution spectra obtained by the IUE
satellite.

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