The ionization structure of the ring nebula. I - Sulfur and argon

Details The ionization structure of the ring nebula. I - Sulfur and argon The ionization structure of the ring nebula. I - Sulfur and argon

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...240...99b&link_type=abstract

Astrophysical Journal, Part 1, vol. 240, Aug. 15, 1980, p. 99-104.

Astronomy and Astrophysics

Astrophysics

59

Argon, Gas Ionization, Line Spectra, Planetary Nebulae, Spectral Energy Distribution, Sulfur, Abundance, Gas Density, Gas Temperature, Image Dissector Tubes, Stellar Mass, Tables (Data), Telescopes, Wavelengths

Scientific paper

Measurements of line intensities in the Ring Nebula have been made in four of the six positions observed by Hawley and Miller over a wider wavelength range. The conclusions of Hawley and Miller about the physical conditions and ionization of He, O, Ne, and N are generally confirmed. New observations of S and Ar line intensities have been made, and new ionization correction formulae for these elements are examined.

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