scholarly journals Theoretical Study of Transition Probabilities and Stark Broadening Parameters and of Several Spectral Lines with Astrophysical Interest of Double-ionized Thallium

2019 ◽  
Vol 870 (2) ◽  
pp. 131 ◽  
Author(s):  
I. de Andrés-García ◽  
C. Colón-Ruiz ◽  
C. Colón
2016 ◽  
Vol 462 (4) ◽  
pp. 4220-4226
Author(s):  
I. de Andrés-García ◽  
C. You ◽  
A. Alonso-Medina ◽  
C. Colón

Author(s):  
Pascal Quinet

AbstractWe present an overview of the advances made during the past 15 years by the Atomic Physics and Astrophysics Group of Mons University regarding the analysis of the spectra, the transition probabilities, and the radiative lifetimes in heavy elements. More precisely, this review is focused on neutral and lowly ionized atoms belonging to the lanthanide group, the fifth row, and the sixth row of the periodic table (Z = 37–86), for which a very large amount of new data has been obtained.


2019 ◽  
Vol 490 (2) ◽  
pp. 1734-1737
Author(s):  
C Moreno-Díaz ◽  
A Alonso-Medina

ABSTRACT 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 4400 Å as well as 7600 Å 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 (τnl) 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).


2003 ◽  
Vol 400 (2) ◽  
pp. 791-793 ◽  
Author(s):  
M. S. Dimitrijević ◽  
M. Dačić ◽  
Z. Cvetković ◽  
S. Sahal-Bréchot

2017 ◽  
Vol 470 (2) ◽  
pp. 2179-2189 ◽  
Author(s):  
C. Colón ◽  
C. Moreno-Díaz ◽  
I. de Andrés-García ◽  
A. Alonso-Medina

Sign in / Sign up

Export Citation Format

Share Document