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Time-dependent atomic diffusion in the atmospheres of CP stars. A big step forward: introducing numerical models including a stellar mass-loss

  • Published:2018-11-10 Issue:4 Volume:482 Page:4519-4527
  • ISSN:0035-8711
  • Container-title:Monthly Notices of the Royal Astronomical Society
  • language:en
  • Short-container-title:

Author:

Alecian G1,Stift M J23

Affiliation:

1. LUTH, Observatoire de Paris, PSL Research University, CNRS, Université Paris Diderot, 5 place Jules Janssen, F-92190 Meudon, France

2. Armagh Observatory, College Hill, Armagh BT61 9DG, UK

3. Kuffner-Sternwarte, Johann Staud-Strasse 10, A-1160 Wien, Austria

Funder

Grand Équipement National De Calcul Intensif

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference38 articles.

1. The Variability of the Hgiiλ3984 Line of the Mercury‐Manganese Star α Andromedae

2. ASP Conf. Ser;Alecian,2012

3. ASP Conf. Ser;Alecian,2013

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1. High-velocity CP2 stars in the Galactic halo;Astronomy & Astrophysics;2023-06

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4. Diffusion velocity of metals in Ap star atmospheres: the effect of ambipolar diffusion of H;Monthly Notices of the Royal Astronomical Society;2023-01-09

5. Analysis of eight magnetic chemically peculiar stars with rotational modulation;Monthly Notices of the Royal Astronomical Society;2022-09-30
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