Experimental and theoretical radiative decay rates for highly excited ruthenium atomic levels and the solar abundance of ruthenium
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Fivet, V
Quinet, P
Palmeri, P
Biemont, E
Asplund, Martin
Grevesse, N
Sauval, A J
Engstrom, L
Lundberg, H
Hartman, H
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Blackwell Publishing Ltd
Abstract
The solar photospheric abundance of ruthenium is revised on the basis of a new set of oscillator strengths derived for Ru i transitions with wavelengths in the spectral range 2250-4710 Å. The new abundance value (in the usual logarithmic scale where the
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Monthly Notices of the Royal Astronomical Society
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Restricted until
2037-12-31
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