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- W1518541702 abstract "Transition probabilities of 100 Ti-II emission lines, originating from 7 different atomic levels, have been determined by combining branching fractions with radiative lifetimes. The branching fractions were measured using Fourier transform spectroscopy on a hollow cathode. The radiative lifetimes of these 7―and 35 additional―levels were measured using time resolved laser-induced fluorescence on a slow Ti ion beam. The transition probabilities of 21 very weak lines have been used to derive a solar titanium abundance of a Ti = log(N Ti /N H ) + 12 = 5.04 ± 0.04 dex, which is insensitive to the solar model. This value is in disagreement with the meteoritic titanium abundance (4.93 ± 0.02)" @default.
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- W1518541702 date "1993-06-01" @default.
- W1518541702 modified "2023-09-23" @default.
- W1518541702 title "Ti-ii transition probabilities and radiative lifetimes in TI and the solar titanium abundance" @default.
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