Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...308..322k&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 308, Sept. 1, 1986, p. 322-336.
Astronomy and Astrophysics
Astrophysics
97
Electron Energy, Forbidden Transitions, Planetary Nebulae, Spectral Energy Distribution, Helium, Interstellar Extinction, Ionization, Line Spectra, Nitrogen, Oxygen Spectra
Scientific paper
Electron temperatures for 107 planetary nebulae are calculated with the most recent atomic parameters from [O III] or [N II] line intensities or both taken from a variety of sources. A detailed investigation of the dependence of the two temperatures on the nebular excitation and on the O/H ratio is presented. Combination of the [O III] and [N II] data sets shows that the mean ratio of Te[N II]/Te[O III] varies smoothly and strongly as a function of overall nebular excitation.
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