Detection of forbidden S III fine-structure emission in ionized nebulae

Details Detection of forbidden S III fine-structure emission in ionized nebulae Detection of forbidden S III fine-structure emission in ionized nebulae

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...213l..71g&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 213, Apr. 15, 1977, p. L71-L74.

Astronomy and Astrophysics

Astrophysics

40

Abundance, Fine Structure, Ionized Gases, Line Spectra, Nebulae, Sulfur, Electron Density (Concentration), Electron Energy, Forbidden Transitions, Infrared Detectors, Infrared Spectra, Luminous Intensity

Scientific paper

The 3P2-3P1 fine-structure line of doubly ionized sulfur has been
detected at 534.41 + or - 0.03 kaysers in the spectra of NGC 7027, BD
+30 deg 3639, and G333.6-0.2. The abundance of S(2+) and the electron
density are discussed. The ionization of G333.6-0.2 is lower than
expected from its luminosity.

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