Atomic diffusion in the atmospheres of upper main-sequence stars
Author:
Publisher
EDP Sciences
Subject
General Engineering,Astronomy and Astrophysics,Space and Planetary Science
Link
http://www.eas-journal.org/10.1051/eas/1363025/pdf
Reference12 articles.
1. The Variability of the Hgiiλ3984 Line of the Mercury‐Manganese Star α Andromedae
2. Alecian G., 2013, in Progress in Solar/Stellar Physics with Helio- and Asteroseismology, Fujihara Seminar, Hakone Nov. 2012, in press
3. Radiative accelerations in stars: The effects of magnetic polarisation revisited
4. Modelling element distributions in the atmospheres of magnetic Ap stars
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1. Distribution of Elements Inside Stars;Communications of the Byurakan Astrophysical Observatory;2019
2. Statistical analysis from recent abundance determinations in HgMn stars;Monthly Notices of the Royal Astronomical Society;2016-04-26
3. Time-dependent atomic diffusion in magnetic ApBp stars;Monthly Notices of the Royal Astronomical Society;2016-01-19
4. Physical Processes Leading to Surface Inhomogeneities: The Case of Rotation;Cartography of the Sun and the Stars;2016
5. Abundance analysis, spectral variability, and search for the presence of a magnetic field in the typical PGa star HD 19400;Monthly Notices of the Royal Astronomical Society;2014-07-03
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