Li I spectra in the 4.65–8.33 micron range: high-L states and oscillator strengths

Context. Infrared (IR) astronomy capacities have rapidly developed in recent years thanks to several ground- and space-based facilities. To take advantage of these capabilities efficiently, a large amount of atomic data (such as line wavenumber, excited-level energy values, and oscillator strengths)...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2012-09, Vol.545, p.A61
Hauptverfasser:	Civiš, S., Ferus, M., Kubelík, P., Chernov, V. E., Zanozina, E. M.
Format:	Artikel
Sprache:	eng
Schlagworte:	atomic data infrared: general line: identification methods: laboratory techniques: spectroscopic
Online-Zugang:	Volltext
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