Memorias de investigación
Artículos en revistas:
Theoretical transition probabilities, radiative lifetimes and Stark broadening parameters of singly ionized magnesium
Año:2019
Áreas de investigación
  • Fisica am -- fisica atomica y molecular,
  • Ingenierías
Datos
Descripción
The presence of spectral lines of singly ionized magnesium (Mg II) in stellar atmospheres has been reported in different stars. Recently, the low-resolution spectrum obtained from Supernova 2014 J in M82, in which Mg II absorption lines centred on 4400Å as well as 7600Å stand out, has been analysed. This is the motive for the atomic data calculations in this work, which are of much interest in the astrophysical area. In this article, ab initio relativistic Hartree?Fock calculations in an intermediate coupling formalism using Cowan?s code allowed us to obtain the required transition probabilities to calculate the theoretical radiative lifetimes for excited nS?, nP?, nD? and nF? states of singly ionized magnesium. An asymptotic dependence of lifetime (? nl) on the effective principal quantum number (n?) has been determined. Also, the Griem semi-empirical approach was used to obtain the theoretical Stark parameters (width and shift) of spectral lines; these data are displayed for an electron density of 1017 cm?3 and temperatures T = 10?100 (×103 K). We have compared the results of lifetimes for 16 levels and Stark parameters for seven spectral lines with previously reported experiments available in the literature. Finally,we discuss the behaviour of the Stark parameters versus temperature for three relevant spectral lines (2802.70, 2797.99 and 7868.04 Å).
Internacional
Si
JCR del ISI
Si
Título de la revista
Mon. Not. Roy. Astron. Soc
ISSN
0035-8711
Factor de impacto JCR
Información de impacto
Volumen
490
DOI
10.1093/mnras/stz2744
Número de revista
Desde la página
1734
Hasta la página
1737
Mes
JULIO
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Participantes
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  • Creador: Departamento: Ingeniería Eléctrica, Electrónica Automática y Física Aplicada