Atomic Transition Probabilities in TiI

Details Atomic Transition Probabilities in TiI Atomic Transition Probabilities in TiI

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aps..dmp..op04n&link_type=abstract

American Physical Society, DAMOP Meeting, 27-30 May 1998 Santa Fe, New Mexico, abstract #OP.04

Astronomy and Astrophysics

Astrophysics

Scientific paper

We report the measurement of branching fractions and atomic transition probabilities for 92 lines connected to high lying, even parity levels in neutral TiI. Branching fractions are determined from six high current hollow cathode emission spectra recorded using the Fourier transform spectrometer at the National Solar Observatory. The absolute scale for normalizing the branching fractions is established using radiative lifetimes from recently-reported time-resolved laser-induced fluorescence measurements.(S. Salih and J. E. Lawler, Astronomy and Astrophysics 239, 407 (1990).) Most of our reported transition probabilities are accurate to better than ±10%.

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