|
|||||
|
|
Stark broadening of B IV lines for astrophysical and laboratory plasma research |
|
| Authors: | Milan S Dimitrijević Magdalena Christova Zoran Simić Andjelka Kovačević Sylvie Sahal-Bréchot |
| Institution: | 1. Astronomical Observatory, Volgina 7, 11060 Belgrade 38, Serbia;2. Laboratoire d’Étude du Rayonnement et de la Matière en Astrophysique, Observatoire de Paris, UMR CNRS 8112, UPMC, 5 Place Jules Janssen, 92195 Meudon Cedex, France;3. Department of Applied Physics, Technical University-Sofia, 1000 Sofia, Bulgaria;4. Faculty of Mathematics, University of Belgrade, 11000 Belgrade, Serbia |
| Abstract: | Stark broadening parameters for 36 multiplets of B IV have been calculated using the semi-classical perturbation formalism. Obtained results have been used to investigate the regularities within spectral series and temperature dependence. |
| Keywords: | Atomic data Atomic processes Line: profiles Stars: atmospheres |
| 本文献已被 ScienceDirect 等数据库收录！ | |