Hyperfine splitting of [Al vi] 3.66 μm and the Al isotopic ratio in NGC 6302
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/359/4/1386/3263043/359-4-1386.pdf
Reference33 articles.
1. Hyperfine Structure in the Solar Spectrum
2. Detection of highly ionized silicon in the planetary nebulae NGC 6302 and NGC 6537
3. A Search for Radioactive 26 Al in the Nova-like Variable V4332 Sagittarii
4. First results from the UHRF: ultra-high-resolution observations of atomic interstellar lines towards ζ Ophiuchi
5. The effect of hyperfine structure on stellar abundance analysis
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1. Study of coupled-cluster correlations on electromagnetic transitions and hyperfine structure constants of W VI;Journal of Physics B: Atomic, Molecular and Optical Physics;2017-05-25
2. Atomic processes in planetary nebulae and H ii regions;Physica Scripta;2009-05
3. DIVISION XII / COMMISSION 14 / WORKING GROUP ATOMIC DATA;Proceedings of the International Astronomical Union;2008-12
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