Absolute transition probabilities in vanadium I and the solar abundance of vanadium

Details Absolute transition probabilities in vanadium I and the solar abundance of vanadium Absolute transition probabilities in vanadium I and the solar abundance of vanadium

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...153..109w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 153, no. 1, Dec. 1985, p. 109-115.

Astronomy and Astrophysics

Astrophysics

47

Abundance, Solar Spectra, Sun, Transition Probabilities, Vanadium, Emission Spectra, Hyperfine Structure, Laser Induced Fluorescence, Spectral Line Width

Scientific paper

The radiative lifetimes of 39 levels in V I have been measured by the method of laser-induced fluorescence from sputtered metal vapor. Emission branching ratios have been measured for these levels to determine absolute transition probabilities for 208 lines in the wavelength range 3180 Å to 16,400 Å. These transition probabilities are used together with high quality solar spectra to derive an improved solar abundance of vanadium, AV = 3.99±0.01. Hyperfine structure effects were included in the abundance calculation.

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