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Theoretical study of the Stark width and shift parameters of Pb III lines: predictions and regularities
Cita
Alonso Medina, Aurelia 
ORCID: https://orcid.org/0000-0002-7460-6561, Colón Hernández, Cristóbal ORCID: https://orcid.org/0000-0003-4663-7122 and Zanón Ballesteros, Antonio ORCID: https://orcid.org/0000-0003-2198-892X
(2008).
Theoretical study of the Stark width and shift parameters of Pb III lines: predictions and regularities.
"Monthly Notices of the Royal Astronomical Society", v. 385
(n. 1);
pp. 261-268.
ISSN 0035-8711.
https://doi.org/10.1111/j.1365-2966.2008.12717.x.
ORCID: https://orcid.org/0000-0002-7460-6561, Colón Hernández, Cristóbal ORCID: https://orcid.org/0000-0003-4663-7122 and Zanón Ballesteros, Antonio ORCID: https://orcid.org/0000-0003-2198-892X
(2008).
Theoretical study of the Stark width and shift parameters of Pb III lines: predictions and regularities.
"Monthly Notices of the Royal Astronomical Society", v. 385
(n. 1);
pp. 261-268.
ISSN 0035-8711.
https://doi.org/10.1111/j.1365-2966.2008.12717.x.
Descripción
| Título: | Theoretical study of the Stark width and shift parameters of Pb III lines: predictions and regularities |
|---|---|
| Autor/es: |
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| Tipo de Documento: | Artículo |
| Título de Revista/Publicación: | Monthly Notices of the Royal Astronomical Society |
| Fecha: | Marzo 2008 |
| ISSN: | 0035-8711 |
| Volumen: | 385 |
| Número: | 1 |
| Materias: | |
| ODS: | |
| Palabras Clave Informales: | Atomic data; Atomic processes |
| Escuela: | E.U.I.T. Industrial (UPM) [antigua denominación] |
| Departamento: | Física Aplicada [hasta 2014] |
| Licencias Creative Commons: | Reconocimiento - Sin obra derivada - No comercial |
Resumen
Semiclassical approximate values of the Stark parameters for several lines of Pb III are reported in this paper. The parameters were calculated using a set of wavefunctions obtained from Hartree–Fock relativistic calculations. Stark widths for 122 lines of Pb III arising from 5d¹⁰6s np (n=6,7,8), 5d¹⁰6s ns (n=7,8,9) and 5d¹⁰6s nd (n = 6,7) configurations have been calculated in this way. Stark widths and shifts are presented as a function of temperature for an electron density of 10¹⁷ cmˉ³. Our results are compared with available experimental data. These atomic data are relevant to the analysis of isotopic abundances of Pb III found in the atmospheres of the star χ Lupy and several subdwarf B and OB stars.
Proyectos asociados
Tipo
Código
Acrónimo
Responsable
Título
Universidad Politécnica de Madrid
CCG06-UPM/FI-229
Sin especificar
Sin especificar
Sin especificar
Comunidad de Madrid
Sin especificar
IV PRICIT
Sin especificar
IV Plan Regional de Investigación Científica e Innovación Tecnológica
Más información
| ID de Registro: | 56539 |
|---|---|
| Identificador DC: | https://oa.upm.es/56539/ |
| Identificador OAI: | oai:oa.upm.es:56539 |
| URL Portal Científico: | https://portalcientifico.upm.es/es/ipublic/item/5482920 |
| Identificador DOI: | 10.1111/j.1365-2966.2008.12717.x |
| URL Oficial: | https://academic.oup.com/mnras/article/385/1/261/1... |
| Depositado por: | Memoria Investigacion |
| Depositado el: | 24 Sep 2019 08:09 |
| Ultima Modificación: | 12 Nov 2025 00:00 |
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