Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008a%26a...492..609n&link_type=abstract
Astronomy and Astrophysics, Volume 492, Issue 2, 2008, pp.609-616
Astronomy and Astrophysics
Astrophysics
5
Atomic Data, Methods: Laboratory, Techniques: Spectroscopic, Line: Identification, Line: Profiles
Scientific paper
We used high-resolution Fourier transform spectroscopy to measure new and improved transition probabilities and hyperfine data for singly ionized niobium. Intensity calibrated spectra were used to measure branching fractions of 145 Nb ii lines in the wavelength interval 2600-4600 Å. Combining the branching fractions with previously reported lifetimes, absolute oscillator strengths for these 145 transitions were derived. In addition, line structures due to magnetic hyperfine interaction were studied resulting in new hyperfine splitting constants for 28 even and 24 odd energy levels.
Ivarsson S.
Nilsson Hampus
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