Revised and extended analysis of five times ionized Xenon, Xe VI

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 probabi...

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Detalles Bibliográficos
Autores principales: Gallardo, Mario O., Raineri, María Mónica, Reyna Almandos, Jorge Guillermo, Pagan, C.J.B., Abrahão, R. A.
Formato: Articulo
Lenguaje:Inglés
Publicado: 2015
Materias:
Física
Atomic data
Line: identification
Ultraviolet: general
White dwarfs
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/86457
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-86457
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Física
Atomic data
Line: identification
Ultraviolet: general
White dwarfs
spellingShingle Física
Atomic data
Line: identification
Ultraviolet: general
White dwarfs
Gallardo, Mario O.
Raineri, María Mónica
Reyna Almandos, Jorge Guillermo
Pagan, C.J.B.
Abrahão, R. A.
Revised and extended analysis of five times ionized Xenon, Xe VI
topic_facet Física
Atomic data
Line: identification
Ultraviolet: general
White dwarfs
description 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.
format Articulo
Articulo
author Gallardo, Mario O.
Raineri, María Mónica
Reyna Almandos, Jorge Guillermo
Pagan, C.J.B.
Abrahão, R. A.
author_facet Gallardo, Mario O.
Raineri, María Mónica
Reyna Almandos, Jorge Guillermo
Pagan, C.J.B.
Abrahão, R. A.
author_sort Gallardo, Mario O.
title Revised and extended analysis of five times ionized Xenon, Xe VI
title_short Revised and extended analysis of five times ionized Xenon, Xe VI
title_full Revised and extended analysis of five times ionized Xenon, Xe VI
title_fullStr Revised and extended analysis of five times ionized Xenon, Xe VI
title_full_unstemmed Revised and extended analysis of five times ionized Xenon, Xe VI
title_sort revised and extended analysis of five times ionized xenon, xe vi
publishDate 2015
url http://sedici.unlp.edu.ar/handle/10915/86457
work_keys_str_mv AT gallardomarioo revisedandextendedanalysisoffivetimesionizedxenonxevi
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AT reynaalmandosjorgeguillermo revisedandextendedanalysisoffivetimesionizedxenonxevi
AT pagancjb revisedandextendedanalysisoffivetimesionizedxenonxevi
AT abrahaora revisedandextendedanalysisoffivetimesionizedxenonxevi
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