• Fulltext


        Click here to view fulltext PDF

      Permanent link:

    • Keywords


      Stark broadening; atomic data; Ne I: line profiles.

    • Abstract


      In order to complete Stark broadening data for Ne I spectral lines which are needed for analysis of stellar atmospheres, collisional widths and shifts (the so-called Stark broadening parameters) of 29 isolated spectral lines of neutral neon have been determined within the impact semiclassical perturbation method. Calculations have been performed for the broadening by collisions with electrons, protons and ionized helium for astrophysical applications, and for collisions with ionized neon and argon for laboratory plasma diagnostics. The shifts have been compared with existing experimental values. The obtained data will be included in the STARK-B database, which is a part of the Virtual Atomic and Molecular Data Center – VAMDC.

    • Author Affiliations


      Milan S. Dimitrijević1 2 3 Zoran Simić1 Andjelka Kovačević4 Aleksandar Valjarević5 Sylvie Sahal-Bréchot2

      1. Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia.
      2. LERMA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universities, UPMC Univ. Paris 06, 5 Place Jules Janssen, 92195 Meudon Cedex, France.
      3. IHIS Techno Experts, Bežanijski put 23, 11080 Belgrade-Zemun, Serbia.
      4. Department of Astronomy, Faculty of Mathematics, Studentski Trg 16, 11000 Belgrade, Serbia.
      5. University of Kosovska Mitrovica, Faculty of Natural Science and Mathematics, Department of Geography, Ive Lole Ribara 29, 38220 Kosovska Mitrovica, Serbia.
    • Dates

  • Journal of Astrophysics and Astronomy | News

    • Continuous Article Publication

      Posted on January 27, 2016

      Since January 2016, the Journal of Astrophysics and Astronomy has moved to Continuous Article Publishing (CAP) mode. This means that each accepted article is being published immediately online with DOI and article citation ID with starting page number 1. Articles are also visible in Web of Science immediately. All these have helped shorten the publication time and have improved the visibility of the articles.

    • Editorial Note on Continuous Article Publication

      Posted on July 25, 2019

      Click here for Editorial Note on CAP Mode

© 2017-2019 Indian Academy of Sciences, Bengaluru.