The apsidal motion in binary stars built on a point-source convective-core model with varying guillotine factor.
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Publication:2584492
DOI10.1086/144330zbMath67.0792.03OpenAlexW1972425734MaRDI QIDQ2584492
Publication date: 1941
Published in: The Astrophysical Journal (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1086/144330
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