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Studies on E2 Transition in the Na-like Highly Stripped Ion Fe XVI

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dc.contributor.author Ray, H
dc.date.accessioned 2008-07-17T07:10:57Z
dc.date.available 2008-07-17T07:10:57Z
dc.date.issued 2002-11
dc.identifier.citation The Astrophysical Journal, Vol. 579, No. 2, pp. 914 – 919 en
dc.identifier.issn 0004-637X
dc.identifier.uri http://hdl.handle.net/2248/2722
dc.description.abstract The spectrum of the solar corona and plasma spectra in astrophysical objects and fusion devices exhibit forbidden lines in alkali-like ions. Ions belonging to the iron group are particularly important in this respect. The electric quadrupole (E2) transitions for Fe XVI are computed using the highly correlated relativistic wave function obtained by using coupled cluster theory including all single, double, and some triple excitations from the core. Term values of the present ion obtained by our method are compared with the available experimental and theoretical data. The detailed highly accurate relativistic data for line strengths and transition probabilities are presented for a large number of transitions of low transition rates, and a few of both of them are compared with existing data as samples. en
dc.format.extent 92998 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher The American Astronomical Society en
dc.relation.uri http://www.journals.uchicago.edu/doi/abs/10.1086/342874 en
dc.subject Atomic Data en
dc.subject Spectrum en
dc.subject Solar Corona en
dc.subject Plasma Spectra en
dc.subject Astrophysical Objects en
dc.subject On-Line Material: Machine-Readable Table en
dc.title Studies on E2 Transition in the Na-like Highly Stripped Ion Fe XVI en
dc.type Article en


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