Abstract
In Sect. 4.2 and Chap. 13 we assumed complete ionization of all atoms. This is a good approximation in the very deep interior, where T and P are sufficiently large, but the degree of ionization certainly becomes smaller if one approaches the stellar surface, where T and P are small.
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Baker, N., Kippenhahn, R. (1962): Z. Astrophys. 54, 114
Cox, A.N. (2000): Allen’s Astrophysical Quantities, 4th edition (Springer, New York)
Saumon, D., Chabrier, G., van Horn, H.M. (1995): Astrophys. J. Suppl. Ser. 99, 713
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Kippenhahn, R., Weigert, A., Weiss, A. (2012). Ionization. In: Stellar Structure and Evolution. Astronomy and Astrophysics Library. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-30304-3_14
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DOI: https://doi.org/10.1007/978-3-642-30304-3_14
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