Measurement and study of rotation in close binary stars (IV) Comparison between observation and predictions of two theories.

Details Measurement and study of rotation in close binary stars (IV) Comparison between observation and predictions of two theories. Measurement and study of rotation in close binary stars (IV) Comparison between observation and predictions of two theories.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996acaps..16..370p&link_type=abstract

Acta Astrophys. Sin., Vol. 16, No. 4, p. 370 - 376

Astronomy and Astrophysics

Astrophysics

Close Binaries: Stellar Rotation

Scientific paper

The author estimates ages of the detached systems in paper (III), calculates characteristic times of synchronization for each "normal" component in the binaries. He compares the age of each component and its theoretical characteristic times of synchronization, analyzes the synchronization property of each star. He concludes that dynamical tide is one of the most effective synchronization mechanisms for the early-type components in close binary systems.

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