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The solar abundance of nickel from photospheric [Niii] lines
Authors:N Grevesse  J P Swings
Institution:(1) Institut d'Astrophysique, Université de Liège, Cointe-Ougrée, Belgium;(2) Joint Institute for Laboratory Astrophysics, Boulder, Colo., U.S.A.
Abstract:The detailed study of the possible presence of four Niii] lines in solar absorption leads to an abundanceA ni = logN ni = 6.30±0.30 (in the usual scale where logN H = 12.00), in agreement with the coronal and meteoritic values.On leave from Institut d'Astrophysique, Université de Liège.
Keywords:
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