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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1466
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dc.contributor.authorSinha, K-
dc.contributor.authorSanwal, B. B-
dc.date.accessioned2007-03-22T05:20:38Z-
dc.date.available2007-03-22T05:20:38Z-
dc.date.issued1992-
dc.identifier.citationBASI, Vol. 20, pp. 283-285en
dc.identifier.urihttp://hdl.handle.net/2248/1466-
dc.description.abstractThe MACKKL photospheric model and the latest oscillator strengths are used to obtain a solar abundance of iron close to the meteoritic value N(Fe) = 7.51 +/- 0.01. This helps to eliminate the discrepancy between photospheric and meteoritic abundances of ironen
dc.format.extent237193 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectSolar atmosphereen
dc.titleOn the solar abundance of ironen
dc.typeArticleen
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