SI III emission line strengths in low density plasmas

Details SI III emission line strengths in low density plasmas SI III emission line strengths in low density plasmas

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.209p...1d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 209, July 1, 1984, p. 1P-4P. Research supported by the

Astronomy and Astrophysics

Astronomy

15

Cosmic Plasma, Emission Spectra, Plasma Spectra, Rarefied Plasmas, Silicon, Ultraviolet Astronomy, Collision Parameters, Planetary Nebulae, Plasma Density, Plasma Diagnostics, Spectral Line Width

Scientific paper

Theoretical emissivity ratios appropriate to homogeneous optically thin
plasmas are presented for the Si III lines at 1883 and 1892 Å.
These lines are a useful density diagnostic for Ne ≥
104cm-3, their use being illustrated for the
planetary nebulae NGC 7662 and V1016 Cygni.

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