Abstract
In lieu of an introduction, we briefly review the observed abundance anomalies that are the main motivation for the study of atomic diffusion in stars, and then early papers which pioneered the field but occasionally reached surprising conclusions.
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Michaud, G., Alecian, G., Richer, J. (2015). Observational Motivation and Brief History. In: Atomic Diffusion in Stars. Astronomy and Astrophysics Library. Springer, Cham. https://doi.org/10.1007/978-3-319-19854-5_1
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DOI: https://doi.org/10.1007/978-3-319-19854-5_1
Publisher Name: Springer, Cham
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