Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..38..301d&link_type=abstract
Astrophysics and Space Science, vol. 38, Dec. 1975, p. 301-312. Fonds de la Recherche Fondamentale Collective
Astronomy and Astrophysics
Astrophysics
18
Binary Stars, Main Sequence Stars, Orbital Elements, Stellar Evolution, Stellar Rotation, X Ray Stars, Circular Orbits, Gyration, Mass Transfer, Pulsars, Radiation Pressure, Stellar Mass, Supernovae, X Ray Binaries, X Ray Sources
Scientific paper
Effects of stellar evolution and tidal interaction on the periods of massive close X-ray binaries during post-supernova evolution are discussed. The orbit is assumed recircularized and synchronized after a certain time. Conditions required in order that tidal forces maintain or restore synchronism are examined. Conditions for collision of the binary system components are also considered. System instability resulting from changes in the structure of the primary, or from transfer of angular momentum from the orbital motion into the rotation or vice versa, are examined. Radiation pressure effects are considered. A test in future observations is stated with respect to circularization of the orbit and tidal evolution.
de Greve Jean-Pierre
de Loore Camiel
Sutantyo W.
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