Chemical abundances of planetary nebulae from optical recombination lines – II. The neon abundance of NGC 7009
By S.-G. Luo, Xunchuan Liu, M. J. Barlow. 2001
193 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science
View Paper: https://www.semanticscholar.org/paper/85357fd2f65ad26cf9ba9375623f3fc0206ca239
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In Astronomy and Astrophysics
- F. Bresolin
- Robert C. Kennicutt Jr.
- Lisa J. Kewley
- D. Garnett
- G. Stasińska
- John Moustakas
- R. Maiolino
- Sara L. Ellison
In Atmospheric Science
Citations in the corpus
- The Composition Gradient in M101 Revisited. II. Electron Temperatures and Implications for the Nebular Abundance Scale (2003, background): “Significant differences between T[O iii] and T(Bac) are observed in planetary nebulae (Liu et al. 2001), but it is not clear whether the two temperatures should be the same, given temperature stratification in ionized nebulae (Stasińska 1978; Garnett 1992).”