IUE spectrum of the IO torus - Identification of the 5S2-3P2,1 transition of S III

Details IUE spectrum of the IO torus - Identification of the 5S2-3P2,1 transition of S III IUE spectrum of the IO torus - Identification of the 5S2-3P2,1 transition of S III

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...275l..19m&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 275, Dec. 1, 1983, p. L19-L23.

Astronomy and Astrophysics

Astrophysics

33

Abundance, Atomic Spectra, Io, Satellite Atmospheres, Sulfur, Ultraviolet Spectra, Atomic Energy Levels, Collision Parameters, Iue, Toroidal Plasmas

Scientific paper

A low-resolution ultraviolet (1150 - 1800 Å) spectrum of the Io torus has been obtained with IUE. Brightness values for emission features due to S+, S++, S+++, and an upper limit for O++ have been determined simultaneously. The splitting in the emission feature near 1729 Å was clearly apparent. The most likely assignment for these lines at 1713.8 Å and 1729.2 Å is the 5S2 → 3P2,1 intercombination doublet which has not been identified in any laboratory or natural source until this time.

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