dc.creatorGallardo M.
dc.creatorRaineri M.
dc.creatorReyna Almandos J.
dc.creatorPagan C.J.B.
dc.creatorAbrahao R.A.
dc.date2015
dc.date2015-06-25T12:55:51Z
dc.date2015-11-26T15:21:50Z
dc.date2015-06-25T12:55:51Z
dc.date2015-11-26T15:21:50Z
dc.date.accessioned2018-03-28T22:31:15Z
dc.date.available2018-03-28T22:31:15Z
dc.identifier
dc.identifierAstrophysical Journal, Supplement Series. Institute Of Physics Publishing, v. 216, n. 1, p. - , 2015.
dc.identifier670049
dc.identifier10.1088/0067-0049/216/1/11
dc.identifierhttp://www.scopus.com/inward/record.url?eid=2-s2.0-84921344952&partnerID=40&md5=6f148b93fa07a90edd8be543186dacb4
dc.identifierhttp://www.repositorio.unicamp.br/handle/REPOSIP/85660
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/85660
dc.identifier2-s2.0-84921344952
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1260297
dc.descriptionA capillary discharge tube was used to record the Xe spectrum in the 400-5500 Å region. A set of 243 lines of the Xe VI spectrum was observed, and 146 of them were classified for the first time. For all known lines, we calculated the weighted oscillator strengths (gf) and weighted transition probabilities (gA) using the configuration interaction in a relativistic Hartree-Fock approach. The energy matrix was calculated using energy parameters adjusted to fit the experimental energy levels. Core polarization effects were taken into account in our calculations. Experimental energy values and calculated lifetimes are also presented for a set of 88 levels. From these levels, 32 were classified for the first time and 33 had their values revised. Our analysis of the 5s5p5d and 5s5p6s configurations was extended in order to clarify discrepancies among previous works.
dc.description216
dc.description1
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dc.languageen
dc.publisherInstitute of Physics Publishing
dc.relationAstrophysical Journal, Supplement Series
dc.rightsaberto
dc.sourceScopus
dc.titleRevised And Extended Analysis Of Five Times Ionized Xenon, Xe Vi
dc.typeArtículos de revistas


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