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Quantum mechanical line widths of ionized oxygen, silicon and aluminium; comparisons with recent experimental results

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  • معلومة اضافية
    • Contributors:
      Umm Al-Qura University; Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA (UMR_8112)); Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris; Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Université de Cergy Pontoise (UCP); Université Paris-Seine-Université Paris-Seine-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS); Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA); École normale supérieure - Paris (ENS-PSL); Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris; Centre National de la Recherche Scientifique (CNRS)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Cergy Pontoise (UCP); Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS)
    • بيانات النشر:
      CCSD
      Oxford University Press (OUP): Policy P - Oxford Open Option A
    • الموضوع:
      2023
    • Collection:
      Archive de l'Observatoire de Paris (HAL)
    • نبذة مختصرة :
      International audience ; We present in this paper new quantum Half Widths at Half intensity Maximum (HWHM) for 101 spectral lines of the following ions: O II (35 lines), O III (20 lines), Si II (9 lines), Si III (12 lines) and Al III (25 lines). The present quantum results are compared to new experimental ones. No previous quantum calculations have been performed for these ions. The relatively high differences found between the new and previous measurements and the available theoretical calculations encourage us to conduct these quantum calculations. Our quantum method has been used many years ago and has given good results compared to other approaches, so it can be a useful tool to check the new experimental results, or to understand the disagreement found for some lines. Furthermore, the obtained results can be used for the abundance determination of elements, the calculation of stellar opacity, the interpretation and modelling of stellar spectra, and the estimation of the relative transfer through stellar plasmas, etc. Part of the present results will be also implemented to the database of Stark broadening parameters STARK-B.
    • الرقم المعرف:
      10.1093/mnras/stad656
    • الدخول الالكتروني :
      https://hal.sorbonne-universite.fr/hal-04024546
      https://hal.sorbonne-universite.fr/hal-04024546v1/document
      https://hal.sorbonne-universite.fr/hal-04024546v1/file/2023-MNRAS_Elabidi-Sahal-Bre%CC%81chot%20et%20al_stad656_preprint.pdf
      https://doi.org/10.1093/mnras/stad656
    • Rights:
      http://hal.archives-ouvertes.fr/licences/copyright/ ; info:eu-repo/semantics/OpenAccess
    • الرقم المعرف:
      edsbas.FCAF4AF