The dissipation factor in contact binaries

Details The dissipation factor in contact binaries The dissipation factor in contact binaries

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...145...25h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 145, no. 1, April 1985, p. 25-40.

Astronomy and Astrophysics

Astrophysics

20

Eclipsing Binary Stars, Energy Dissipation, Light Curve, Radiative Heat Transfer, Stellar Luminosity, Asymptotic Methods, Differential Equations, Equations Of Motion, Mach Number, Newton Second Law, Stellar Winds

Scientific paper

It is argued that a large part of the light emitted from the secondary
components of W UMa stars could have its origin in the dissipation of
mechanical energy. This possibility could indicate the way towards a
resolution of the so-called "light curve paradox" which arises from
attempts to represent the W UMa stars by theoretical models.

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