Abstract
Tidal effects in close binaries are well known as an important source of information on stellar interiors. Such information can also be obtained for a single star if it pulsates, like radial or non-radial pulsating stars. In the last thirty years many different models for the structure and evolution of the stars have been performed.
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© 2000 Springer Science+Business Media Dordrecht
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İbanoğlu, C. (2000). Apsidal Motion in Close Binaries. In: İbanoğlu, C. (eds) Variable Stars as Essential Astrophysical Tools. NATO Science Series, vol 544. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4299-1_28
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DOI: https://doi.org/10.1007/978-94-011-4299-1_28
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