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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Published in | Astronomy and astrophysics (Berlin) Vol. 671; p. A22 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
01.03.2023
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Online Access | Get full text |
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