2001/10/30 by O. G. Benvenuto, Aldo Serenelli, A. M. Serenelli +4 · 1 citation
Physics and Astronomy · #Apsidal precession #Astro and Planetary Science #Astronomical and nuclear sciences #Astronomy #Astrophysics #Binary number #Binary star #Classical mechanics #Motion (physics) #Physics #Planet #Proper motion #Star (game theory) #Stars #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1046/j.1365-8711.2002.05083.x
published as Mon.Not.Roy.Astron.Soc. 330 (2002) 435 · To be published in MNRAS, 7 pages, 8 figures
arxiv created 2001/10/30 · openalex publication_date 2002/02/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The motion of the apse of a binary is mainly a direct consequence of the finite size of its components. If both stars were spherical objects and General Relativity corrections