Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...202l.135p&link_type=abstract
Astrophysical Journal, vol. 202, Dec. 15, 1975, pt. 2, p. L135-L137.
Astronomy and Astrophysics
Astronomy
65
Binary Stars, Radiation Sources, Stellar Rotation, X Ray Astronomy, Eccentricity, Eddy Viscosity, Hydrodynamics, Stellar Structure, Turbulence Effects
Scientific paper
Rotation through a tidal bulge generates a fluid shear which, in stars, implies a very high Reynolds number; fully developed turbulence might result. Turbulent viscosities, synchronization, and circularization time scales are computed. The calculation contains no adjustable dimensional parameters. It explains the observed fact of synchronous rotation for orbital periods not exceeding about 4 days and of nonsynchronous rotation for larger periods. The observed small eccentricity of some short-period binary X-ray sources is also an immediate consequence.
Press William H.
Smarr Larry
Wiita Paul J.
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