Synchronization in early-type close binaries

Details Synchronization in early-type close binaries Synchronization in early-type close binaries

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26as...59...37g&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 59, Jan. 1985, p. 37-42.

Astronomy and Astrophysics

Astrophysics

5

Early Stars, Eclipsing Binary Stars, Stellar Motions, Stellar Rotation, A Stars, Angular Velocity, F Stars, Synchronism

Scientific paper

Extending previous studies, the synchronism between rotation and revolution in early-type (from O to F5) close binaries is discussed. Confirming that a strong tendency to synchronism extends up to pairs wider than usually thought, the present study further specifies that this tendency is stronger in the late A and especially in the F-type stars than in the hotter ones; but in contrast with previous contentions, it does not appear to be stronger in stars evolved from the main sequence (with respect to dwarfs) or in Am stars (with respect to normal stars).

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