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An internally consistent set of oscillator strengths for Fe I lines

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dc.contributor.author Giridhar, S
dc.contributor.author Ferro, A. A
dc.date.accessioned 2008-09-16T14:02:41Z
dc.date.available 2008-09-16T14:02:41Z
dc.date.issued 1989-03
dc.identifier.citation Journal of Astrophysics and Astronomy, Vol. 10, No. 1, pp. 47 - 83 en
dc.identifier.issn 0250-6335
dc.identifier.uri http://hdl.handle.net/2248/3637
dc.description.abstract An extensive set of internally consistent oscillator strength values for Fe I lines is compiled using literature data and scaling the oscillator strengths derived by different workers to that of Blackwell and his coworkers. A relationship is developed that can be used for calculating the gf values for Fe I lines for cases where gf values are not available, and the nature of errors in the gf values that were reported by Kurucz and Peytremann (1975) is examined. The newly calculated gf values are listed, together with the gf values reported by other investigators as well as corrections to be applied to the oscillator strengths of Kurucz and Peytremann (1975) for lines belonging to different multiplets. en
dc.language.iso en en
dc.publisher Indian Academy of Sciences en
dc.relation.uri http://ads.iucaa.ernet.in/abs/1989JApA...10...47G en
dc.subject Iron en
dc.subject Line spectra en
dc.subject Oscillator strengths en
dc.subject Spectrum analysis en
dc.subject Stellar atmospheres en
dc.subject Stellar composition en
dc.subject Abundance en
dc.subject Astronomical spectroscopy en
dc.subject Fine structure en
dc.subject Quantitative analysis en
dc.title An internally consistent set of oscillator strengths for Fe I lines en
dc.type Article en


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