Abstract
Since we do not wish to interrupt the derivation of the energy equation for stars with lengthy formalisms, we first provide a few thermodynamic relations which will be used extensively later on.
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© 1990 Springer-Verlag Berlin Heidelberg
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Kippenhahn, R., Weigert, A. (1990). Conservation of Energy. In: Stellar Structure and Evolution. Astronomy and Astrophysics Library. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-61523-8_4
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DOI: https://doi.org/10.1007/978-3-642-61523-8_4
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-58013-3
Online ISBN: 978-3-642-61523-8
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