Zusammenfassung
Bis jetzt haben wir in der Theorie der Linienprofile nur solche Verbreiterungsursachen berücksichtigt, die in den Sternatmosphären selbst ihren Sitz haben und also direkt den Absorptions- bzw. Streukoeffizienten beeinflussen.
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© 1955 Springer-Verlag Ohg. Berlin · Göttingen · Heidelberg
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Unsöld, A. (1955). Beeinflussung der Linienprofile durch Rotation und Expansion der Sterne. In: Physik der Sternatmosphären. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-47425-5_18
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DOI: https://doi.org/10.1007/978-3-642-47425-5_18
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