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dc.date.accessioned 2019-12-02T13:57:02Z
dc.date.available 2019-12-02T13:57:02Z
dc.date.issued 2015
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/86457
dc.description.abstract A 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. en
dc.language en es
dc.subject Atomic data es
dc.subject Line: identification es
dc.subject Ultraviolet: general es
dc.subject White dwarfs es
dc.title Revised and extended analysis of five times ionized Xenon, Xe VI en
dc.type Articulo es
sedici.identifier.other doi:10.1088/0067-0049/216/1/11 es
sedici.identifier.other eid:2-s2.0-84921344952 es
sedici.identifier.issn 0067-0049 es
sedici.creator.person Gallardo, Mario O. es
sedici.creator.person Raineri, María Mónica es
sedici.creator.person Reyna Almandos, Jorge Guillermo es
sedici.creator.person Pagan, C.J.B. es
sedici.creator.person Abrahão, R. A. es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Centro de Investigaciones Ópticas es
mods.originInfo.place Facultad de Ciencias Exactas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Astrophysical Journal, Supplement Series es
sedici.relation.journalVolumeAndIssue vol. 216, no. 1 es
sedici.rights.sherpa * Color: green * Pre-print del autor: can * Post-print del autor: can * Versión de editor/PDF:can * Condiciones: >>On any website, arXiv, scientific social networks (except Research Gate) or non-commercial open access repository. >>Publisher's version/PDF may be used on any website or authors' institutional repository >>Publisher copyright and source must be acknowledged >>Must link to publisher version >>Publisher's version/PDF may be used >>Authors depositing in arXiv must they choose the first licence statement offered by arXiv when uploading their article � a "non-exclusive licence to distribute" >>Publisher last contacted on 10/02/2016 >>Publisher last reviewed on 15/08/2017 * Link a Sherpa: http://sherpa.ac.uk/romeo/issn/0067-0049/es/


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)