On the solar abundance of iron

dc.contributor.author	Sinha, K.
dc.contributor.author	Sanwal, B. B.
dc.date.accessioned	2010-01-13T10:58:04Z
dc.date.available	2010-01-13T10:58:04Z
dc.date.issued	1992
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/426
dc.description.abstract	Utilizing the MACKKL photospheric model and the latest oscillator strengths, solar abundances of iron close to the meteoritic value N(Fe) = 7.51 ± 0.01 is obtained. It helps to remove the discrepancy between photospheric and meteoritic abundances of iron.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi20-283
dc.subject	Iron abundances , Photospheric models	en_US
dc.title	On the solar abundance of iron	en_US
dc.type	Article	en_US