Transition probabilities in Kr III spectrum, of interest for high resolution stellar spectra analysis

Details Transition probabilities in Kr III spectrum, of interest for high resolution stellar spectra analysis Transition probabilities in Kr III spectrum, of interest for high resolution stellar spectra analysis

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pobeo..75...93d&link_type=abstract

Publications of the Astronomical Observatory of Belgrade (ISSN 0373-3742), No. 75, p. 93 - 96 (2003). In: Proceedings of the XII

Physics

Physics Of Stars, Stellar Systems, Krypton, Synthetic Spectra

Scientific paper

Using the relative line intensity ratio (RLIR) method, transition probability values of the spontaneous emission (Einstein's A values) of 7 transitions in the doubly ionized krypton (Kr III) spectra have been obtained relatively to the reference A value related to the 324.569 nm Kr III, most intensive transition in the Kr III spectra. Our Kr III transition probability values are the first data for this ion obtained experimentally using the RLIR method. Values have been calculated also using the Coulomb approximation (CA) method taking into account new atomic data for Kr III energy levels.

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