Kr II transition probabilities for analysis of trace element lines in high resolution stellar spectra

Details Kr II transition probabilities for analysis of trace element lines in high resolution stellar spectra Kr II transition probabilities for analysis of trace element lines in high resolution stellar spectra

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pobeo..75..111d&link_type=abstract

Publications of the Astronomical Observatory of Belgrade (ISSN 0373-3742), No. 75, p. 111 - 115 (2003). In: Proceedings of the X

Physics

Physics Of Stars, Stellar Systems, Stellar Spectra: Krypton

Scientific paper

On the basis of the relative line intensity ratio (RLIR) method transition probability value for the spontaneous emission (Einstein's values) of 14 transitions in the singly ionized krypton (Kr II) spectra have been obtained relatively to the reference A value related to the 435.548 nm Kr II most intensive transition in the Kr II spectra. Mentioned A values have been calculated also using the Coulomb approximation (CA) method taking into account new atomic data for Kr II energy levels.

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