Theoretical investigation of the occurrence of tidally excited oscillations in massive eccentric binary systems

Context. Massive and intermediate-mass stars reside in binary systems at a much higher rate than low-mass stars. At the same time, binaries containing massive main-sequence (MS) component(s) are often characterised by eccentric orbits, and can therefore be observed as eccentric ellipsoidal variables...

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Bibliographic Details
Published inAstronomy and astrophysics (Berlin) Vol. 671; p. A22
Main Authors Kołaczek-Szymański, P. A., Różański, T.
Format Journal Article
LanguageEnglish
Published 01.03.2023
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