Rotation of close binary system components

Details Rotation of close binary system components Rotation of close binary system components

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.218..223m&link_type=abstract

Astrophysics and Space Science, vol. 218, no. 2, p. 223-248

Astronomy and Astrophysics

Astrophysics

5

Axes Of Rotation, Binary Stars, Inclination, Rotation, Stellar Evolution, Stellar Models, Stellar Orbits, Error Analysis, Graphs (Charts), Gravitational Fields, Stellar Magnitude, Stellar Spectra, Tables (Data)

Scientific paper

The rotation of close binary system components is investigated. The principal physical characteristics as well as the equatorial rotational and the axial and orbital inclinations for 46 close binary systems were determined. It is found that the rotation axes of the individual stars in a pair cross the orbital plane under different angles. As a rule, the rotation and orbital periods of a vast majority of the systems investigated here do not coincide.

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